Research Article Open Access
Effects of Maxwellian ions on Dust-acoustic Solitary Waves in Adiabatic Degenerate Plasmas and It’s Instability
Nushrat Khan, Sharmin Yiasmin Swarna and Md. Masum Haider*
Department of Physics, Mawlana Bhashani Science and Technology University, Santosh, Tangail-1902, Bangla
*Corresponding author: Md. Masum Haider, Department of Physics, Mawlana Bhashani Science and Technology University, Santosh, Tangail-1902, Bangladesh; Email: @/ @
Received: October 11, 2017; Accepted: October 25, 2017; Published: November 23, 2017
Citation: Haider MD, Khan N, et al. (2017) Effects of Maxwellian ions on Dust-acoustic Solitary Waves in Adiabatic Degenerate Plasmas and It’s Instability. Int J Hematol Blo Dis 1(1): 1-8.
Abstract Top
A rigorous theoretical investigation has been made on dust acoustic solitary waves in unmagnetized and magnetized degenerate plasmas with adiabatic pressure. Korteweg-de Vries (K-dV) equation have been derived for unmagnetized case as well as its solution. For the case of magnetized plasmas, Zakharov-Kuznetsov (ZK) equation, and its solution have been derived and studied its instability criterion and growth rate. It has been found that, the parametric regimes effects not only modify the basic properties of dust acoustic solitary waves and its instability criterion but also introduce some important new features.

Keywords: Maxwellian ions; Dust-acoustic Solitary Waves; Degenerate Plasmas; K-dV equation; ZK euation; Instability;
Introduction
The propagation of dust acoustic waves (DASW’s) waves plays an important role in understanding the different behaviour of dust components or different waves phenomena in dusty plasmas which are omnipresent in laboratory, space and astrophysical plasma environments, such as cometary tails, planetary ring, interstellar medium etc. The dust grain changes the nature of the system including the creation of the new modes. In the recent years, many important and precious, theoretical and experimental investigation has been made on solitary waves. DASW’s are one of the most significant non-linear affair in plasma method. Different properties such as amplitude, width etc. of the solitary waves can be modified by using different perturbation method. Bliokh and Yaroshenko studied the elecrostatic waves in dusty plasmas and applied their results in interpreting spoke-like structures in Saturn’s rings (revealed by the voyager space mission)[1, 2]. Rao et.al, were the first to predict theoretically existence of extremely lower phase velocity DASW’s in unmagnetized dusty plasmas whose constituent are inertial charged dust grains and Boltzmann distributed ions and electrons [3]. Roychoudhury and Mukherjee considered a two-component unmagnetized dusty plasma consisting of a negatively charged adiabatic dust fluid and an inertia-less isothermal ion fluid and investigated the effects of dust fluid temperature on large amplitude solitary waves by the pseudo-potential approach [4]. Sayed and Mamun assumed a dusty plasma containing the adiabatic dust fluid and non-adiabatic (isothermal) inertia-less electron and ion fluid and studied the effect of the dust fluid temperature on the DASW’s by the reductive perturbation method [5, 6]. Mendoza-Briceño et al, assumed a two-component dusty plasma containing the adiabatic dust fluid and non-adiabatic ions following the nonthermal distribution of Cairns et al and studied the effect of the dust fluid temperature on the DA solitary waves by the pseudo-potential approach [7-9].

The equation of state for degenerate electrons in such intersteller compact objects are mathematically explained by Chandrasekhar for two limits, namely non-relativistic and ultrarelativistic limits [10,11]. The degenerate electron equation of state of Chandrasekhar is p e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiCamaaBa aaleaacaWGLbaabeaaaaa@3800@ is proportional to N e 5/3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOtamaaDa aaleaacaWGLbaabaGaaGynaiaac+cacaaIZaaaaaaa@3A0E@ for the non-relativistic limit and p e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiCamaaBa aaleaacaWGLbaabeaaaaa@3800@ is proportional to N e 4/3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOtamaaDa aaleaacaWGLbaabaGaaGynaiaac+cacaaIZaaaaaaa@3A0E@ the ultrarelativistic limit where p e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiCamaaBa aaleaacaWGLbaabeaaaaa@3800@ is the degenerate electron pressure and N e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOtamaaBa aaleaacaWGLbaabeaaaaa@37DE@ is the degenerate electron number density. Mamun and Shukla considered an unmagnetized degenerate plasma without and with negatively charged stationary dust [12, 13]. Mamun et al, studied the ion acoustic Solitary Waves (SW’s) in the presence of an external magnetic field for ultra-relativistic degenerate electron-ion plasmas using the reductive perturbation technique [14]. Using the same technique Haider et al, also studied the obliquely propagating solitary structure with the presence of external magnetic field [15,16]. But the presence of heavy ions, which can be arbitrary charged, were not considered in the work of Mamun et al and Haider et al [14,15].

In the present work we have studied the nonlinear propagation of DA SW’s in unmagnetized and magnetized degenerate plasmas with adiabatic pressure. We have studied both ultra-relativistic and non-relativistic case simultaneously using the generalized equation proposed by Haider [17]. To do this we have derived Korteweg-de Vries (K-dV) and Zakharov-Kuznetsov (ZK) equation by reductive perturbation method and find out the solution of it [6]. We have studied the instability criterion as well as it’s growth rate.
Plasma Model
We have studied the nonlinear propagation of DASW’s in unmagnetized and magnetized degenerate plasmas for adiabatic situation containing,

(i) inertial positive mobile dust component
(ii) inertialess degenerate electrons
(iii) inertialess degenerate positrons
(iv) stationary negative dust component
(v) inertial Maxwellian ions

At equilibrium, we have, n pd0 + n i0 + n p0 = n nd0 + n e0    (1) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGWbGaamizaiaaicdaaeqaaOGaey4kaSIaamOBamaaBaaa leaacaWGPbGaaGimaaqabaGccqGHRaWkcaWGUbWaaSbaaSqaaiaadc hacaaIWaaabeaakiabg2da9iaad6gadaWgaaWcbaGaamOBaiaadsga caaIWaaabeaakiabgUcaRiaad6gadaWgaaWcbaGaamyzaiaaicdaae qaaOGaaeiiaiaabccacaqGGaGaaeikaiaabgdacaqGPaaaaa@4D8B@ where, n pd0 ,  n i0 , n p0 , n nd0 ,  n e0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGWbGaamizaiaaicdaaeqaaOGaaiilaiaabccacaWGUbWa aSbaaSqaaiaadMgacaaIWaaabeaakiaacYcacaaMe8UaamOBamaaBa aaleaacaWGWbGaaGimaaqabaGccaGGSaGaaGjbVlaad6gadaWgaaWc baGaamOBaiaadsgacaaIWaaabeaakiaacYcacaqGGaGaamOBamaaBa aaleaacaWGLbGaaGimaaqabaaaaa@4D01@ are the positive dust, ion, positron, negative dust and electron number densities at equilibrium respectively.
Solitary Waves in Unmagnetized Plasmas
Basic Equations
The dynamics of such DASW’s in one dimensional form and is given by the followings equations, n pd t + x ( n pd u pd )=0     (2) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacq GHciITcaWGUbWaaSbaaSqaaiaadchacaWGKbaabeaaaOqaaiabgkGi 2kaadshaaaGaey4kaSYaaSaaaeaacqGHciITaeaacqGHciITcaWG4b aaaiaacIcacaWGUbWaaSbaaSqaaiaadchacaWGKbaabeaakiaadwha daWgaaWcbaGaamiCaiaadsgaaeqaaOGaaiykaiabg2da9iaaicdaca qGGaGaaeiiaiaabccacaqGGaGaaeiiaiaabIcacaqGYaGaaeykaaaa @4FF5@ u pd t +( u pd x ) u pd = φ x ( σ d n pd ) x p pd      (3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacq GHciITcaWG1bWaaSbaaSqaaiaadchacaWGKbaabeaaaOqaaiabgkGi 2kaadshaaaGaey4kaSIaaiikaiaadwhadaWgaaWcbaGaamiCaiaads gaaeqaaOWaaSaaaeaacqGHciITaeaacqGHciITcaWG4baaaiaacMca caWG1bWaaSbaaSqaaiaadchacaWGKbaabeaakiabg2da9iabgkHiTm aalaaabaGaeyOaIyRaeqOXdOgabaGaeyOaIyRaamiEaaaacqGHsisl caGGOaWaaSaaaeaacqaHdpWCdaWgaaWcbaGaamizaaqabaaakeaaca WGUbWaaSbaaSqaaiaadchacaWGKbaabeaaaaGccaqGPaWaaSaaaeaa cqGHciITaeaacqGHciITcaWG4baaaiaadchadaWgaaWcbaGaamiCai aadsgaaeqaaOGaaeiiaiaabccacaqGGaGaaeiiaiaabccacaqGOaGa ae4maiaabMcaaaa@64ED@ u pd t +( u pd x ) p pd +α p pd x u pd = 0    (4) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacq GHciITcaWG1bWaaSbaaSqaaiaadchacaWGKbaabeaaaOqaaiabgkGi 2kaadshaaaGaey4kaSIaaiikaiaadwhadaWgaaWcbaGaamiCaiaads gaaeqaaOWaaSaaaeaacqGHciITaeaacqGHciITcaWG4baaaiaacMca caWGWbWaaSbaaSqaaiaadchacaWGKbaabeaakiaabUcacqaHXoqyca WGWbWaaSbaaSqaaiaadchacaWGKbaabeaakmaalaaabaGaeyOaIyla baGaeyOaIyRaamiEaaaacaWG1bWaaSbaaSqaaiaadchacaWGKbaabe aakiaab2dacaqGGaGaaeimaiaabccacaqGGaGaaeiiaiaabccacaqG OaGaaeinaiaabMcaaaa@5BF0@ 2 φ x 2 =( μ e n e μ p n p n pd μ i n i + μ nd n nd )      (5) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacq GHciITdaahaaWcbeqaaiaaikdaaaGccqaHgpGAaeaacqGHciITcaWG 4bWaaWbaaSqabeaacaaIYaaaaaaakiabg2da9iaacIcacqaH8oqBda WgaaWcbaGaamyzaaqabaGccaWGUbWaaSbaaSqaaiaadwgaaeqaaOGa eyOeI0IaeqiVd02aaSbaaSqaaiaadchaaeqaaOGaamOBamaaBaaale aacaWGWbaabeaakiabgkHiTiaad6gadaWgaaWcbaGaamiCaiaadsga aeqaaOGaeyOeI0IaeqiVd02aaSbaaSqaaiaadMgaaeqaaOGaamOBam aaBaaaleaacaWGPbaabeaakiabgUcaRiabeY7aTnaaBaaaleaacaWG UbGaamizaaqabaGccaWGUbWaaSbaaSqaaiaad6gacaWGKbaabeaaki aacMcacaqGGaGaaeiiaiaabccacaqGGaGaaeiiaiaabccacaqGOaGa aeynaiaabMcaaaa@6207@ where, n pd MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGWbGaamizaaqabaaaaa@38F2@ is the positive dust number density normalized by its equilibrium value n pd0 ,  n nd MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGWbGaamizaiaaicdaaeqaaOGaaiilaiaabccacaWGUbWa aSbaaSqaaiaad6gacaWGKbaabeaaaaa@3E04@ is the negative dust number density normalized by its equilibrium value n nd0 ,  n p MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGUbGaamizaiaaicdaaeqaaOGaaiilaiaabccacaWGUbWa aSbaaSqaaiaadchaaeqaaaaa@3D1B@ is the positron number density normalized by its equilibrium value n p0 ,  n i MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGWbGaaGimaaqabaGccaGGSaGaaeiiaiaad6gadaWgaaWc baGaamyAaaqabaaaaa@3C2D@ is the ion number density normalized by its equilibrium value n i0 ,  n e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGPbGaaGimaaqabaGccaGGSaGaaeiiaiaad6gadaWgaaWc baGaamyzaaqabaaaaa@3C22@ is the electron number density normalized by its equilibrium value n e0 ,  u pd MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGLbGaaGimaaqabaGccaGGSaGaaeiiaiaadwhadaWgaaWc baGaamiCaiaadsgaaeqaaaaa@3D19@ is the dust fluid speed normalized by C pd = ( m nd c 2 / m pd ) 1/2 ,  m pd MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4qamaaBa aaleaacaWGWbGaamizaaqabaGccqGH9aqpcaGGOaGaamyBamaaBaaa leaacaWGUbGaamizaaqabaGccaWGJbWaaWbaaSqabeaacaaIYaaaaO Gaai4laiaad2gadaWgaaWcbaGaamiCaiaadsgaaeqaaOGaaiykamaa CaaaleqabaGaaGymaiaac+cacaaIYaaaaOGaaiilaiaabccacaWGTb WaaSbaaSqaaiaadchacaWGKbaabeaaaaa@4A78@ is the rest mass of positive dust, m nd MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyBamaaBa aaleaacaWGUbGaamizaaqabaaaaa@38EF@ is the mass of negative dust and C being the speed of light. φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ is the DA electrostatic wave potential normalized by ( m pd C pd 2 / z d e) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGikaiaad2 gadaWgaaWcbaGaamiCaiaadsgaaeqaaOGaam4qamaaDaaaleaacaWG WbGaamizaaqaaiaaikdaaaGccaaIVaGaamOEamaaBaaaleaacaWGKb aabeaakiaadwgacaaIPaaaaa@41BA@ , with z d MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOEamaaBa aaleaacaWGKbaabeaaaaa@3809@ is the number of positive charge residing on the positive charged dust and e being the magnitude of unit charge. α MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdegaaa@3794@ is the adiabatic index. σ d MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4Wdm3aaS baaSqaaiaadsgaaeqaaaaa@38CD@ is the ratio of the positive dust temperature to negative dust temperature. μ e = n e0 / n pd0 ,  μ p = n p0 / n pd0 μ i = n i0 / n pd0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaOGaaGypaiaad6gadaWgaaWcbaGaamyzaiaa icdaaeqaaOGaaG4laiaad6gadaWgaaWcbaGaamiCaiaadsgacaaIWa aabeaakiaacYcacaqGGaGaeqiVd02aaSbaaSqaaiaadchaaeqaaOGa aGypaiaad6gadaWgaaWcbaGaamiCaiaaicdaaeqaaOGaaG4laiaad6 gadaWgaaWcbaGaamiCaiaadsgacaaIWaaabeaakiaabYcacaqGGaGa eqiVd02aaSbaaSqaaiaadMgaaeqaaOGaaGypaiaad6gadaWgaaWcba GaamyAaiaaicdaaeqaaOGaaG4laiaad6gadaWgaaWcbaGaamiCaiaa dsgacaaIWaaabeaaaaa@595A@ and μ nd = n nd0 / n pd0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaad6gacaWGKbaabeaakiaai2dacaWGUbWaaSbaaSqaaiaa d6gacaWGKbGaaGimaaqabaGccaaIVaGaamOBamaaBaaaleaacaWGWb Gaamizaiaaicdaaeqaaaaa@42B3@

Here the space variables are normalized by Debye radius λ d = ( m pd c 2 /4π n d0 z d 2 e 2 ) 1/2 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4UdW2aaS baaSqaaiaadsgaaeqaaOGaeyypa0Jaaiikaiaad2gadaWgaaWcbaGa amiCaiaadsgaaeqaaOGaam4yamaaCaaaleqabaGaaGOmaaaakiaac+ cacaaI0aGaeqiWdaNaamOBamaaBaaaleaacaWGKbGaaGimaaqabaGc caWG6bWaa0baaSqaaiaadsgaaeaacaaIYaaaaOGaamyzamaaCaaale qabaGaaGOmaaaakiaacMcadaahaaWcbeqaaiaaigdacaGGVaGaaGOm aaaaaaa@4D11@ and time variable (t) is normalized by ω pd 1 = ( m pd /4π n pd0 z d 2 e 2 ) 1/2 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdC3aa0 baaSqaaiaadchacaWGKbaabaGaeyOeI0IaaGymaaaakiabg2da9iaa cIcacaWGTbWaaSbaaSqaaiaadchacaWGKbaabeaakiaac+cacaaI0a GaeqiWdaNaamOBamaaBaaaleaacaWGWbGaamizaiaaicdaaeqaaOGa amOEamaaDaaaleaacaWGKbaabaGaaGOmaaaakiaadwgadaahaaWcbe qaaiaaikdaaaGccaGGPaWaaWbaaSqabeaacaaIXaGaai4laiaaikda aaaaaa@4EE2@ .

Non-thermal distributed ions can be represented by, n i =(1φ+ 1 2 φ 2 )     (6) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGPbaabeaakiaai2dacaaIOaGaaGymaiabgkHiTiabeA8a QjabgUcaRmaalaaabaGaaGymaaqaaiaaikdaaaGaeqOXdO2aaWbaaS qabeaacaaIYaaaaOGaaGykaiaabccacaqGGaGaaeiiaiaabccacaqG GaGaaeikaiaabAdacaqGPaaaaa@47F5@ According to Haider the value of n e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGLbaabeaaaaa@37FE@ and n p MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGWbaabeaaaaa@3809@ can be express respectively as [18, 19], n e = (1+ γ1 β φ) 1 γ1     (7) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGLbaabeaakiabg2da9iaacIcacaaIXaGaey4kaSYaaSaa aeaacqaHZoWzcqGHsislcaaIXaaabaGaeqOSdigaaiabeA8aQjaacM cadaahaaWcbeqaamaalaaabaGaaGymaaqaaiabeo7aNjabgkHiTiaa igdaaaaaaOGaaeiiaiaabccacaqGGaGaaeiiaiaabIcacaqG3aGaae ykaaaa@4BAF@ and      n p = (1 γ1 β φ) 1 γ1       (8) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyyaiaad6 gacaWGKbGaaeiiaiaabccacaqGGaGaaeiiaiaabccacaWGUbWaaSba aSqaaiaadchaaeqaaOGaeyypa0JaaiikaiaaigdacqGHsisldaWcaa qaaiabeo7aNjabgkHiTiaaigdaaeaacqaHYoGyaaGaeqOXdOMaaiyk amaaCaaaleqabaWaaSaaaeaacaaIXaaabaGaeq4SdCMaeyOeI0IaaG ymaaaaaaGccaqGGaGaaeiiaiaabccacaqGGaGaaeiiaiaabccacaqG OaGaaeioaiaabMcaaaa@52FD@ where, β=( K E ) n 0 (γ1) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaiIcadaWcaaqaaiaadUeaaeaacaWGfbaaaiaaiMcacaWGUbWa a0baaSqaaiaaicdaaeaacaaIOaGaeq4SdCMaeyOeI0IaaGymaiaaiM caaaaaaa@41FA@ , where, K= 1 18(γ1)  ( 3 Δ 3 π )   (γ1)  E MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4saiaai2 dadaWcaaqaaiaaigdaaeaacaaIXaGaaGioaiaaiIcacqaHZoWzcqGH sislcaaIXaGaaGykaaaacaqGGaGaaGikamaalaaabaGaaG4maiabfs 5aenaaCaaaleqabaGaaG4maaaaaOqaaiabec8aWbaacaaIPaGaaeii amaaCaaaleqabaGaaGikaiabeo7aNjabgkHiTiaaigdacaaIPaaaaO Gaaeiiaiaadweaaaa@4C6F@ with Λ(= h m pd c ) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeu4MdWKaaG ikaiaai2dadaWcaaqaaiaadIgaaeaacaWGTbWaaSbaaSqaaiaadcha caWGKbaabeaakiaadogaaaGaaGykaaaa@3E81@ is the Compton wavelength normalized by Debye radious ( λ d ), E= m pd c 2 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeU 7aSnaaBaaaleaacaWGKbaabeaakiaacMcacaGGSaGaaeiiaiaadwea caaI9aGaamyBamaaBaaaleaacaWGWbGaamizaaqabaGccaWGJbWaaW baaSqabeaacaaIYaaaaaaa@41DC@ and n 0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaaIWaaabeaaaaa@37CE@ be the number density of plasma particle. γ=4/3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4SdCMaaG ypaiaaisdacaaIVaGaaG4maaaa@3A97@ for ultra-relativistic case and γ=5/3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4SdCMaaG ypaiaaiwdacaaIVaGaaG4maaaa@3A98@ for nonrelativistic case.
K-dV Equation
We now follow the reductive perturbation method and construct a weakly nonlinear theory for the DA waves with small but finite amplitude, which leads to a scaling of the independent variables through the stretched coordinates as [6, 18, 19],
Z= ε 1/2  (x v p t)     (9) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOwaiaai2 dacqaH1oqzdaahaaWcbeqaaiaaigdacaaIVaGaaGOmaaaakiaabcca caaIOaGaamiEaiabgkHiTiaadAhadaWgaaWcbaGaamiCaaqabaGcca WG0bGaaGykaiaabccacaqGGaGaaeiiaiaabccacaqGGaGaaeikaiaa bMdacaqGPaaaaa@47FC@ τ= ε 3/2  t    (10) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiXdqNaaG ypaiabew7aLnaaCaaaleqabaGaaG4maiaai+cacaaIYaaaaOGaaeii aiaadshacaqGGaGaaeiiaiaabccacaqGGaGaaeikaiaabgdacaqGWa Gaaeykaaaa@4377@
where, ε MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyTdugaaa@379C@ is a smallness parameter measuring the weakness of the dispersion, v p MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamODamaaBa aaleaacaWGWbaabeaaaaa@3811@ is the nonlinear wave phase velocity. We can expand the perturbed quantities n pd ,  u pd ,  p pd MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGWbGaamizaaqabaGccaGGSaGaaeiiaiaadwhadaWgaaWc baGaamiCaiaadsgaaeqaaOGaaiilaiaabccacaWGWbWaaSbaaSqaai aadchacaWGKbaabeaaaaa@41AF@ and φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ bout their equilibrium values in powers of ε MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyTdugaaa@379C@ ,
n pd =1+ε n pd (1) + ε 2 n pd (2) +...    (11) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGWbGaamizaaqabaGccaaI9aGaaGymaiabgUcaRiabew7a Ljaad6gadaqhaaWcbaGaamiCaiaadsgaaeaacaaIOaGaaGymaiaaiM caaaGccqGHRaWkcqaH1oqzdaahaaWcbeqaaiaaikdaaaGccaWGUbWa a0baaSqaaiaadchacaWGKbaabaGaaGikaiaaikdacaaIPaaaaOGaey 4kaSIaaGOlaiaai6cacaaIUaGaaeiiaiaabccacaqGGaGaaeiiaiaa bIcacaqGXaGaaeymaiaabMcaaaa@5329@ u pd =0+ε u pd (1) + ε 2 u pd (2) +...     (12) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyDamaaBa aaleaacaWGWbGaamizaaqabaGccaaI9aGaaGimaiabgUcaRiabew7a LjaadwhadaqhaaWcbaGaamiCaiaadsgaaeaacaaIOaGaaGymaiaaiM caaaGccqGHRaWkcqaH1oqzdaahaaWcbeqaaiaaikdaaaGccaWG1bWa a0baaSqaaiaadchacaWGKbaabaGaaGikaiaaikdacaaIPaaaaOGaey 4kaSIaaGOlaiaai6cacaaIUaGaaeiiaiaabccacaqGGaGaaeiiaiaa bccacaqGOaGaaeymaiaabkdacaqGPaaaaa@53E1@ φ=0+ε φ (1) + ε 2 φ (2) +...    (13) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOMaaG ypaiaaicdacqGHRaWkcqaH1oqzcqaHgpGAdaahaaWcbeqaaiaaiIca caaIXaGaaGykaaaakiabgUcaRiabew7aLnaaCaaaleqabaGaaGOmaa aakiabeA8aQnaaCaaaleqabaGaaGikaiaaikdacaaIPaaaaOGaey4k aSIaaGOlaiaai6cacaaIUaGaaeiiaiaabccacaqGGaGaaeiiaiaabI cacaqGXaGaae4maiaabMcaaaa@4FB8@ p pd =1+ε p pd (1) + ε 2 p pd (2) +...    (14) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiCamaaBa aaleaacaWGWbGaamizaaqabaGccaaI9aGaaGymaiabgUcaRiabew7a LjaadchadaqhaaWcbaGaamiCaiaadsgaaeaacaaIOaGaaGymaiaaiM caaaGccqGHRaWkcqaH1oqzdaahaaWcbeqaaiaaikdaaaGccaWGWbWa a0baaSqaaiaadchacaWGKbaabaGaaGikaiaaikdacaaIPaaaaOGaey 4kaSIaaGOlaiaai6cacaaIUaGaaeiiaiaabccacaqGGaGaaeiiaiaa bIcacaqGXaGaaeinaiaabMcaaaa@5332@
Using the stretched coordinates and equations (11)-(14) in equations (2)-(5); and equating the coefficients of ε 3/2 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyTdu2aaW baaSqabeaacaaIZaGaaG4laiaaikdaaaaaaa@39FB@ from the continuity and momentum equation and coefficients of ε MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyTdugaaa@379C@ from Poisson’s equation and rearranging the parameters one can obtain the linear dispersion relation for the DASW’s
v p = 1 ( 1 β μ e + 1 β μ p + μ i ) +α σ d       (15) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamODamaaBa aaleaacaWGWbaabeaakiaai2dadaGcaaqaamaalaaabaGaaGymaaqa aiaaiIcadaWcaaqaaiaaigdaaeaacqaHYoGyaaGaeqiVd02aaSbaaS qaaiaadwgaaeqaaOGaey4kaSYaaSaaaeaacaaIXaaabaGaeqOSdiga aiabeY7aTnaaBaaaleaacaWGWbaabeaakiabgUcaRiabeY7aTnaaBa aaleaacaWGPbaabeaakiaaiMcaaaGaey4kaSIaeqySdeMaeq4Wdm3a aSbaaSqaaiaadsgaaeqaaaqabaGccaqGGaGaaeiiaiaabccacaqGGa GaaeiiaiaabccacaqGOaGaaeymaiaabwdacaqGPaaaaa@5647@
It can be seen from equation (15) that the presence of the Maxwellian ions significantly modifies the linear dispersion relation.

Equating the next higher order co-efficient of from above equations and using the parameters we can finally obtain a K-dV equation describing the nonlinear propagation of the DASW’s in the dusty plasma
Figure 1: A=0 graph, showing the variation of β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdigaaa@3796@ with μ e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaaaa@38C1@ and μ p MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadchaaeqaaaaa@38CC@ for the values of α=0.5,  μ i =0.4 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGynaiaacYcacaqGGaGaeqiVd02aaSbaaSqa aiaadMgaaeqaaOGaaGypaiaaicdacaaIUaGaaGinaaaa@41B0@ and γ=5/3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4SdCMaaG ypaiaaiwdacaaIVaGaaG4maaaa@3A98@
Figure 2: A=0 graph, showing the variation of β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdigaaa@3796@ with μ e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaaaa@38C1@ and μ p MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadchaaeqaaaaa@38CC@ for the values of α=0.5,  μ i =0.4 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGynaiaacYcacaqGGaGaeqiVd02aaSbaaSqa aiaadMgaaeqaaOGaaGypaiaaicdacaaIUaGaaGinaaaa@41B0@ and γ=4/3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4SdCMaaG ypaiaaiwdacaaIVaGaaG4maaaa@3A98@
φ (1) τ +A φ (1)   φ (1) Z +B 3 φ (1) Z 3 =0      (16) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacq GHciITcqaHgpGAdaahaaWcbeqaaiaaiIcacaaIXaGaaGykaaaaaOqa aiabgkGi2kabes8a0baacqGHRaWkcaWGbbGaeqOXdO2aaWbaaSqabe aacaaIOaGaaGymaiaaiMcaaaGccaqGGaWaaSaaaeaacqGHciITcqaH gpGAdaahaaWcbeqaaiaaiIcacaaIXaGaaGykaaaaaOqaaiabgkGi2k aadQfaaaGaey4kaSIaamOqamaalaaabaGaeyOaIy7aaWbaaSqabeaa caaIZaaaaOGaeqOXdO2aaWbaaSqabeaacaaIOaGaaGymaiaaiMcaaa aakeaacqGHciITcaWGAbWaaWbaaSqabeaacaaIZaaaaaaakiaai2da caaIWaGaaeiiaiaabccacaqGGaGaaeiiaiaabccacaqGGaGaaeikai aabgdacaqG2aGaaeykaaaa@604F@
where A=[ μ i ( μ e μ p )( 2γ β 2 ) ] ( v p 2 α σ d ) 2 2 v p      (17) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyqaiaai2 dadaWadaqaaiabeY7aTnaaBaaaleaacaWGPbaabeaakiabgkHiTiaa iIcacqaH8oqBdaWgaaWcbaGaamyzaaqabaGccqGHsislcqaH8oqBda WgaaWcbaGaamiCaaqabaGccaaIPaGaaGikamaalaaabaGaaGOmaiab gkHiTiabeo7aNbqaaiabek7aInaaCaaaleqabaGaaGOmaaaaaaGcca aIPaaacaGLBbGaayzxaaWaaSaaaeaacaaIOaGaamODamaaDaaaleaa caWGWbaabaGaaGOmaaaakiabgkHiTiabeg7aHjabeo8aZnaaBaaale aacaWGKbaabeaakiaaiMcadaahaaWcbeqaaiaaikdaaaaakeaacaaI YaGaamODamaaBaaaleaacaWGWbaabeaaaaGccaqGGaGaaeiiaiaabc cacaqGGaGaaeiiaiaabIcacaqGXaGaae4naiaabMcaaaa@602C@ B= ( v p 2 α σ d ) 2 2 v p      (18) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiyBaiaac+ gacaGGKbGaaGymaiaad2gacaWGTbGaamOqaiaai2dadaWcaaqaaiaa iIcacaWG2bWaa0baaSqaaiaadchaaeaacaaIYaaaaOGaeyOeI0Iaeq ySdeMaeq4Wdm3aaSbaaSqaaiaadsgaaeqaaOGaaGykamaaCaaaleqa baGaaGOmaaaaaOqaaiaaikdacaWG2bWaaSbaaSqaaiaadchaaeqaaa aakiaabccacaqGGaGaaeiiaiaabccacaqGGaGaaeikaiaabgdacaqG 4aGaaeykaaaa@507E@
Solution of K-dV Equation
The stationary solution of this K-dV equation can be obtained by transforming the independent variables ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ and τ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiXdqhaaa@37BA@ to ξ=Z u 0 τ, τ=t MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGNaaG ypaiaadQfacqGHsislcaWG1bWaaSbaaSqaaiaaicdaaeqaaOGaeqiX dqNaaiilaiaabccacqaHepaDcaaI9aGaamiDaaaa@42D2@ where u 0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyDamaaBa aaleaacaaIWaaabeaaaaa@37D5@ is a constant solitary wave velocity. For simplicity, we have write φ (1) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdO2aaW baaSqabeaacaaIOaGaaGymaiaaiMcaaaaaaa@39FF@ as φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ . Now using the appropriate boundary conditions for localized disturbances, viz. φ (1) 0, (d φ (1)  /dξ)0, ( d 2 φ (1)  /d ξ 2 )0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdO2aaW baaSqabeaacaaIOaGaaGymaiaaiMcaaaGccqGHsgIRcaaIWaGaaiil aiaabccacaaIOaGaamizaiabeA8aQnaaCaaaleqabaGaaGikaiaaig dacaaIPaaaaOGaaeiiaiaai+cacaWGKbGaeqOVdGNaaGykaiabgkzi UkaaicdacaGGSaGaaeiiaiaaiIcacaWGKbWaaWbaaSqabeaacaaIYa aaaOGaeqOXdO2aaWbaaSqabeaacaaIOaGaaGymaiaaiMcaaaGccaqG GaGaaG4laiaadsgacqaH+oaEdaahaaWcbeqaaiaaikdaaaGccaaIPa GaeyOKH4QaaGimaaaa@5B5E@ at ξ± MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGNaey OKH4QaeyySaeRaeyOhIukaaa@3D04@ . Thus, one can express the stationary solution of this K-dV equation as φ= φ m sec h 2 [ξ/Δ]      (19) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOMaaG ypaiabeA8aQnaaBaaaleaacaWGTbaabeaakiaadohacaWGLbGaam4y aiaadIgadaahaaWcbeqaaiaaikdaaaGccaaIBbGaeqOVdGNaaG4lai abfs5aejaai2facaqGGaGaaeiiaiaabccacaqGGaGaaeiiaiaabcca caqGOaGaaeymaiaabMdacaqGPaaaaa@4C4F@ where φ m =(3 u 0 /A) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdO2aaS baaSqaaiaad2gaaeqaaOGaaGypaiaaiIcacaaIZaGaamyDamaaBaaa leaacaaIWaaabeaakiaai+cacaWGbbGaaGykaaaa@3F2C@ is the amplitude and Δ= 4B u 0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeuiLdqKaaG ypamaakaaabaWaaSaaaeaacaaI0aGaamOqaaqaaiaadwhadaWgaaWc baGaaGimaaqabaaaaaqabaaaaa@3BA7@ is the width of the solitary waves. The value of A and B are shown in (17) and (18) respectively.
Figure 3: Variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for the values of α=0.5, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGynaiaacYcaaaa@3B3C@ μ p =1, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadchaaeqaaOGaaGypaiaaigdacaGGSaaaaa@3B08@ μ i =0.4,  u 0 =0.1, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadMgaaeqaaOGaaGypaiaaicdacaaIUaGaaGinaiaacYca caqGGaGaamyDamaaBaaaleaacaaIWaaabeaakiaai2dacaaIWaGaaG OlaiaaigdacaGGSaaaaa@42A7@ μ e =1.2,  σ d =1, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaOGaaGypaiaaigdacaaIUaGaaGOmaiaacYca caqGGaGaeq4Wdm3aaSbaaSqaaiaadsgaaeqaaOGaaGypaiaaigdaca GGSaaaaa@4228@ β=1, γ=5/3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaigdacaGGSaGaaeiiaiabeo7aNjaai2dacaaI1aGaaG4laiaa iodaaaa@3F0E@ (solid curve) and γ=4/3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4SdCMaaG ypaiaaisdacaaIVaGaaG4maaaa@3A97@ (dotted curve).
Figure 4: Variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for the values of α=0.5,  μ p =1,  μ i =0.4,  μ e =1.2,  u 0 =0.1,  σ d =1, β=0.8 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGynaiaacYcacaqGGaGaeqiVd02aaSbaaSqa aiaadchaaeqaaOGaaGypaiaaigdacaGGSaGaaeiiaiabeY7aTnaaBa aaleaacaWGPbaabeaakiaai2dacaaIWaGaaGOlaiaaisdacaGGSaGa aeiiaiabeY7aTnaaBaaaleaacaWGLbaabeaakiaai2dacaaIXaGaaG OlaiaaikdacaGGSaGaaeiiaiaadwhadaWgaaWcbaGaaGimaaqabaGc caaI9aGaaGimaiaai6cacaaIXaGaaiilaiaabccacqaHdpWCdaWgaa WcbaGaamizaaqabaGccaaI9aGaaGymaiaacYcacaqGGaGaeqOSdiMa aGypaiaaicdacaaIUaGaaGioaaaa@605C@ (Black), β=0.9 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaicdacaaIUaGaaGyoaaaa@3A92@ (Blue) and β=1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaigdaaaa@3918@ (Red). Here dotted curve represented ultra-relativistic (γ=4/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI0aGaaG4laiaaiodacaGGPaaaaa@3BF0@ case and solid curve represented non-relativistic (γ=5/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI1aGaaG4laiaaiodacaGGPaaaaa@3BF1@ case.
Solitary Waves in Magnetized Plasmas
Basic Equations
We have been considered that, there an external static magnetic field present B 0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOqamaaBa aaleaacaaIWaaabeaaaaa@37A2@ acting along the z-direction ( B 0 = k ^ B 0 ) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiaadk eadaWgaaWcbaGaaGimaaqabaGccaaI9aGabm4AayaajaGaamOqamaa BaaaleaacaaIWaaabeaakiaaiMcaaaa@3C89@ where k ^ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGabm4Aayaaja aaaa@36F5@ is the unit vector along the z-direction, so that the ions and dusts are moving along the magnetic field direction.

The dynamics of such DASW’s in three dimensional form and is given by the followings equations, n pd t +.( n pd u pd )=0    (20) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacq GHciITcaWGUbWaaSbaaSqaaiaadchacaWGKbaabeaaaOqaaiabgkGi 2kaadshaaaGaey4kaSIaey4bIeTaaGOlaiaaiIcacaWGUbWaaSbaaS qaaiaadchacaWGKbaabeaakiaadwhadaWgaaWcbaGaamiCaiaadsga aeqaaOGaaGykaiaai2dacaaIWaGaaeiiaiaabccacaqGGaGaaeiiai aabIcacaqGYaGaaeimaiaabMcaaaa@4E37@ u pd t +( u pd .) u pd =.φ+ ω cd ( u pd × k ^ ) ( σ d n pd ) p pd          (21) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGceaqabeaadaWcaa qaaiabgkGi2kaadwhadaWgaaWcbaGaamiCaiaadsgaaeqaaaGcbaGa eyOaIyRaamiDaaaacqGHRaWkcaaIOaGaamyDamaaBaaaleaacaWGWb GaamizaaqabaGccaaIUaGaey4bIeTaaGykaiaadwhadaWgaaWcbaGa amiCaiaadsgaaeqaaOGaaGypaiabgkHiTiabgEGirlaai6cacqaHgp GAcqGHRaWkcqaHjpWDdaWgaaWcbaGaam4yaiaadsgaaeqaaOGaaGik aiaadwhadaWgaaWcbaGaamiCaiaadsgaaeqaaOGaey41aqRabm4Aay aajaGaaGykaaqaaiaaywW7caaMf8UaaiyBaiaac+gacaGGKbGaaGym aiaadogacaWGTbGaeyOeI0IaaGikamaalaaabaGaeq4Wdm3aaSbaaS qaaiaadsgaaeqaaaGcbaGaamOBamaaBaaaleaacaWGWbGaamizaaqa baaaaOGaaGykaiabgEGirlaadchadaWgaaWcbaGaamiCaiaadsgaae qaaOGaaeiiaiaabccacaqGGaGaaeiiaiaabccacaqGGaGaaeiiaiaa bccacaqGGaGaaeikaiaabkdacaqGXaGaaeykaaaaaa@7741@ p pd t +( u pd .) p pd +α p pd . u pd =0      (22) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacq GHciITcaWGWbWaaSbaaSqaaiaadchacaWGKbaabeaaaOqaaiabgkGi 2kaadshaaaGaey4kaSIaaGikaiaadwhadaWgaaWcbaGaamiCaiaads gaaeqaaOGaaGOlaiabgEGirlaaiMcacaWGWbWaaSbaaSqaaiaadcha caWGKbaabeaakiabgUcaRiabeg7aHjaadchadaWgaaWcbaGaamiCai aadsgaaeqaaOGaey4bIeTaaGOlaiaadwhadaWgaaWcbaGaamiCaiaa dsgaaeqaaOGaaGypaiaaicdacaqGGaGaaeiiaiaabccacaqGGaGaae iiaiaabccacaqGOaGaaeOmaiaabkdacaqGPaaaaa@5A59@ 2 φ=( μ e n e μ p n p n pd μ i n i + μ nd   n nd )     (23) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaey4bIe9aaW baaSqabeaacaaIYaaaaOGaeqOXdOMaaGypaiaaiIcacqaH8oqBdaWg aaWcbaGaamyzaaqabaGccaWGUbWaaSbaaSqaaiaadwgaaeqaaOGaey OeI0IaeqiVd02aaSbaaSqaaiaadchaaeqaaOGaamOBamaaBaaaleaa caWGWbaabeaakiabgkHiTiaad6gadaWgaaWcbaGaamiCaiaadsgaae qaaOGaeyOeI0IaeqiVd02aaSbaaSqaaiaadMgaaeqaaOGaamOBamaa BaaaleaacaWGPbaabeaakiabgUcaRiabeY7aTnaaBaaaleaacaWGUb GaamizaaqabaGccaqGGaGaamOBamaaBaaaleaacaWGUbGaamizaaqa baGccaaIPaGaaeiiaiaabccacaqGGaGaaeiiaiaabccacaqGOaGaae OmaiaabodacaqGPaaaaa@5F41@ Here, ω cd MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdC3aaS baaSqaaiaadogacaWGKbaabeaaaaa@39BF@ is the positive dust cyclotron frequency ( z d e B 0 / m pd0 c) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGikaiaadQ hadaWgaaWcbaGaamizaaqabaGccaWGLbGaamOqamaaBaaaleaacaaI Waaabeaakiaai+cacaWGTbWaaSbaaSqaaiaadchacaWGKbGaaGimaa qabaGccaWGJbGaaGykaaaa@417A@ normalized by ω pd =( 4π n pd0   z d 2   e 2 m pd )   1 2 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdC3aaS baaSqaaiaadchacaWGKbaabeaakiaai2dacaaIOaWaaSaaaeaacaaI 0aGaeqiWdaNaamOBamaaBaaaleaacaWGWbGaamizaiaaicdaaeqaaO GaaeiiaiaadQhadaqhaaWcbaGaamizaaqaaiaaikdaaaGccaqGGaGa amyzamaaCaaaleqabaGaaGOmaaaaaOqaaiaad2gadaWgaaWcbaGaam iCaiaadsgaaeqaaaaakiaaiMcacaqGGaWaaWbaaSqabeaadaWcaaqa aiaaigdaaeaacaaIYaaaaaaaaaa@4DA9@
Figure 5: Variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for the values of β=1,  μ p =1,  μ i =0.4,  μ e =1.2,  u 0 =0.1,  σ d =1, α=0.3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaigdacaGGSaGaaeiiaiabeY7aTnaaBaaaleaacaWGWbaabeaa kiaai2dacaaIXaGaaiilaiaabccacqaH8oqBdaWgaaWcbaGaamyAaa qabaGccaaI9aGaaGimaiaai6cacaaI0aGaaiilaiaabccacqaH8oqB daWgaaWcbaGaamyzaaqabaGccaaI9aGaaGymaiaai6cacaaIYaGaai ilaiaabccacaWG1bWaaSbaaSqaaiaaicdaaeqaaOGaaGypaiaaicda caaIUaGaaGymaiaacYcacaqGGaGaeq4Wdm3aaSbaaSqaaiaadsgaae qaaOGaaGypaiaaigdacaGGSaGaaeiiaiabeg7aHjaai2dacaaIWaGa aGOlaiaaiodaaaa@5EE1@ (Black), α=0.4 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGinaaaa@3A8B@ (Red) and α=0.5 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGynaaaa@3A8C@ (Blue). Here dotted curve represented ultra-relativistic (γ=4/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI0aGaaG4laiaaiodacaGGPaaaaa@3BF0@ case and solid curve represented non-relativistic (γ=5/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI1aGaaG4laiaaiodacaGGPaaaaa@3BF1@
Figure 6: Variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for the values of β=1, α=0.5,  μ p =1,  μ i =0.4,  u 0 =0.1,  μ e =1.2,  σ d =0.6 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaigdacaGGSaGaaeiiaiabeg7aHjaai2dacaaIWaGaaGOlaiaa iwdacaGGSaGaaeiiaiabeY7aTnaaBaaaleaacaWGWbaabeaakiaai2 dacaaIXaGaaiilaiaabccacqaH8oqBdaWgaaWcbaGaamyAaaqabaGc caaI9aGaaGimaiaai6cacaaI0aGaaiilaiaabccacaWG1bWaaSbaaS qaaiaaicdaaeqaaOGaaGypaiaaicdacaaIUaGaaGymaiaacYcacaqG GaGaeqiVd02aaSbaaSqaaiaadwgaaeqaaOGaaGypaiaaigdacaaIUa GaaGOmaiaacYcacaqGGaGaeq4Wdm3aaSbaaSqaaiaadsgaaeqaaOGa aGypaiaaicdacaaIUaGaaGOnaaaa@605A@ (Black), σ d =0.8 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4Wdm3aaS baaSqaaiaadsgaaeqaaOGaaGypaiaaicdacaaIUaGaaGioaaaa@3BD2@ (Red) and σ d =1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4Wdm3aaS baaSqaaiaadsgaaeqaaOGaaGypaiaaigdaaaa@3A59@ (Blue). Here dotted curve represented ultra-relativistic (γ=4/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI0aGaaG4laiaaiodacaGGPaaaaa@3BF0@ case and solid curve represented non-relativistic (γ=5/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI1aGaaG4laiaaiodacaGGPaaaaa@3BF1@ case.
Zakharov-Kuznetsov Equation
To derive the Zakharov-Kuznetsov equation, which is known as `K-dV equation in three dimensions’, we first introduce the following stretched coordinates X= ε 1/2  x     (24) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiwaiaai2 dacqaH1oqzdaahaaWcbeqaaiaaigdacaaIVaGaaGOmaaaakiaabcca caWG4bGaaeiiaiaabccacaqGGaGaaeiiaiaabccacaqGOaGaaeOmai aabsdacaqGPaaaaa@4339@ Y= ε 1/2  y      (25) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamywaiaai2 dacqaH1oqzdaahaaWcbeqaaiaaigdacaaIVaGaaGOmaaaakiaabcca caWG5bGaaeiiaiaabccacaqGGaGaaeiiaiaabccacaqGGaGaaeikai aabkdacaqG1aGaaeykaaaa@43DF@ Z= ε 1/2  (z v p t)     (26) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOwaiaai2 dacqaH1oqzdaahaaWcbeqaaiaaigdacaaIVaGaaGOmaaaakiaabcca caaIOaGaamOEaiabgkHiTiaadAhadaWgaaWcbaGaamiCaaqabaGcca WG0bGaaGykaiaabccacaqGGaGaaeiiaiaabccacaqGGaGaaeikaiaa bkdacaqG2aGaaeykaaaa@48B0@ τ= ε 3/2  t     (27) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiXdqNaaG ypaiabew7aLnaaCaaaleqabaGaaG4maiaai+cacaaIYaaaaOGaaeii aiaadshacaqGGaGaaeiiaiaabccacaqGGaGaaeiiaiaabIcacaqGYa Gaae4naiaabMcaaaa@4422@ We can expand the perturbed quantities n pd ,  u pdx ,  u pdy ,  u pdz ,  p pd MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGWbGaamizaaqabaGccaGGSaGaaeiiaiaadwhadaWgaaWc baGaamiCaiaadsgacaWG4baabeaakiaacYcacaqGGaGaamyDamaaBa aaleaacaWGWbGaamizaiaadMhaaeqaaOGaaiilaiaabccacaWG1bWa aSbaaSqaaiaadchacaWGKbGaamOEaaqabaGccaGGSaGaaeiiaiaadc hadaWgaaWcbaGaamiCaiaadsgaaeqaaaaa@4D6B@ and φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ about their equilibrium values in powers of ε MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyTdugaaa@379C@
n pd =1+ε n pd (1) + ε 2 n pd (2) +...      (28) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBamaaBa aaleaacaWGWbGaamizaaqabaGccaaI9aGaaGymaiabgUcaRiabew7a Ljaad6gadaqhaaWcbaGaamiCaiaadsgaaeaacaaIOaGaaGymaiaaiM caaaGccqGHRaWkcqaH1oqzdaahaaWcbeqaaiaaikdaaaGccaWGUbWa a0baaSqaaiaadchacaWGKbaabaGaaGikaiaaikdacaaIPaaaaOGaey 4kaSIaaGOlaiaai6cacaaIUaGaaeiiaiaabccacaqGGaGaaeiiaiaa bccacaqGGaGaaeikaiaabkdacaqG4aGaaeykaaaa@5477@ u pdx =0+ ε 3/2 u pdx (1) + ε 2 u pdx (2) +...      (29) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyDamaaBa aaleaacaWGWbGaamizaiaadIhaaeqaaOGaaGypaiaaicdacqGHRaWk cqaH1oqzdaahaaWcbeqaaiaaiodacaaIVaGaaGOmaaaakiaadwhada qhaaWcbaGaamiCaiaadsgacaWG4baabaGaaGikaiaaigdacaaIPaaa aOGaey4kaSIaeqyTdu2aaWbaaSqabeaacaaIYaaaaOGaamyDamaaDa aaleaacaWGWbGaamizaiaadIhaaeaacaaIOaGaaGOmaiaaiMcaaaGc cqGHRaWkcaaIUaGaaGOlaiaai6cacaqGGaGaaeiiaiaabccacaqGGa GaaeiiaiaabccacaqGOaGaaeOmaiaabMdacaqGPaaaaa@59EC@ u pdy =0+ ε 3/2 u pdy (1) + ε 2 u pdy (2) +...    (30) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbiqaaaDbcaWG1b WaaSbaaSqaaiaadchacaWGKbGaamyEaaqabaGccaaI9aGaaGimaiab gUcaRiabew7aLnaaCaaaleqabaGaaG4maiaai+cacaaIYaaaaOGaam yDamaaDaaaleaacaWGWbGaamizaiaadMhaaeaacaaIOaGaaGymaiaa iMcaaaGccqGHRaWkcqaH1oqzdaahaaWcbeqaaiaaikdaaaGccaWG1b Waa0baaSqaaiaadchacaWGKbGaamyEaaqaaiaaiIcacaaIYaGaaGyk aaaakiabgUcaRiaai6cacaaIUaGaaGOlaiaabccacaqGGaGaaeiiai aabccacaqGOaGaae4maiaabcdacaqGPaaaaa@5979@ u pdz =0+ε u pdz (1) + ε 2 u pdz (2) +...       (31) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyDamaaBa aaleaacaWGWbGaamizaiaadQhaaeqaaOGaaGypaiaaicdacqGHRaWk cqaH1oqzcaWG1bWaa0baaSqaaiaadchacaWGKbGaamOEaaqaaiaaiI cacaaIXaGaaGykaaaakiabgUcaRiabew7aLnaaCaaaleqabaGaaGOm aaaakiaadwhadaqhaaWcbaGaamiCaiaadsgacaWG6baabaGaaGikai aaikdacaaIPaaaaOGaey4kaSIaaGOlaiaai6cacaaIUaGaaeiiaiaa bccacaqGGaGaaeiiaiaabccacaqGGaGaaeiiaiaabIcacaqGZaGaae ymaiaabMcaaaa@5825@ φ=0+ε φ (1) + ε 2 φ (2) +...     (32) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOMaaG ypaiaaicdacqGHRaWkcqaH1oqzcqaHgpGAdaahaaWcbeqaaiaaiIca caaIXaGaaGykaaaakiabgUcaRiabew7aLnaaCaaaleqabaGaaGOmaa aakiabeA8aQnaaCaaaleqabaGaaGikaiaaikdacaaIPaaaaOGaey4k aSIaaGOlaiaai6cacaaIUaGaaeiiaiaabccacaqGGaGaaeiiaiaabc cacaqGOaGaae4maiaabkdacaqGPaaaaa@505C@ p pd =1+ε p pd (1) + ε 2 p pd (2) +...    (33) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiCamaaBa aaleaacaWGWbGaamizaaqabaGccaaI9aGaaGymaiabgUcaRiabew7a LjaadchadaqhaaWcbaGaamiCaiaadsgaaeaacaaIOaGaaGymaiaaiM caaaGccqGHRaWkcqaH1oqzdaahaaWcbeqaaiaaikdaaaGccaWGWbWa a0baaSqaaiaadchacaWGKbaabaGaaGikaiaaikdacaaIPaaaaOGaey 4kaSIaaGOlaiaai6cacaaIUaGaaeiiaiaabccacaqGGaGaaeiiaiaa bIcacaqGZaGaae4maiaabMcaaaa@5333@
Figure 7: Variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for the values of β=1, α=0.5,  μ i =0.4,  u 0 =0.1,  μ e =1.2,  σ d =1,  μ p =0.8 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaigdacaGGSaGaaeiiaiabeg7aHjaai2dacaaIWaGaaGOlaiaa iwdacaGGSaGaaeiiaiabeY7aTnaaBaaaleaacaWGPbaabeaakiaai2 dacaaIWaGaaGOlaiaaisdacaGGSaGaaeiiaiaadwhadaWgaaWcbaGa aGimaaqabaGccaaI9aGaaGimaiaai6cacaaIXaGaaiilaiaabccacq aH8oqBdaWgaaWcbaGaamyzaaqabaGccaaI9aGaaGymaiaai6cacaaI YaGaaiilaiaabccacqaHdpWCdaWgaaWcbaGaamizaaqabaGccaaI9a GaaGymaiaacYcacaqGGaGaeqiVd02aaSbaaSqaaiaadchaaeqaaOGa aGypaiaaicdacaaIUaGaaGioaaaa@605C@ (Blue), μ p =0.9 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadchaaeqaaOGaaGypaiaaicdacaaIUaGaaGyoaaaa@3BD2@ (Black) and μ p =1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadchaaeqaaOGaaGypaiaaigdaaaa@3A58@ (Red). Here dotted curve represented ultra-relativistic (γ=4/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI0aGaaG4laiaaiodacaGGPaaaaa@3BF0@ case and solid curve represented non-relativistic (γ=5/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI1aGaaG4laiaaiodacaGGPaaaaa@3BF1@ case.
Next, substituting eqs. (24)-(33) into eqs. (20)-(23) and obtain the lowest order equations of (20)-(23) which in turn can be solved as (15), the linear dispersion relation for DASW’s. This implies that linear dispersion relation for unmagnetized and magnetized situations are same. Magnetic field does not effect on the linear dispersion relation.

Equating the next higher order co-efficient of ε MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyTdugaaa@379C@ from above equations and by the use of parameters we can finally obtained ZK equation describing the nonlinear propagation of the DA SW’s in the dusty plasma φ (1) τ +PQ φ (1)   φ (1) Z MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7caGGTbGaai4BaiaacsgacqGHsislcaaIXaGaam4yaiaad2gadaWc aaqaaiabgkGi2kabeA8aQnaaCaaaleqabaGaaGikaiaaigdacaaIPa aaaaGcbaGaeyOaIyRaeqiXdqhaaiabgUcaRiaadcfacaWGrbGaeqOX dO2aaWbaaSqabeaacaaIOaGaaGymaiaaiMcaaaGccaqGGaWaaSaaae aacqGHciITcqaHgpGAdaahaaWcbeqaaiaaiIcacaaIXaGaaGykaaaa aOqaaiabgkGi2kaadQfaaaaaaa@5727@ + 1 2 P Z [ 2 Z 2 +R( 2 X 2 + 2 Y 2 ) ] φ (1)  =0      (34) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7cqGHRaWkdaWcaaqaaiaaigdaaeaacaaIYaaaaiaadcfadaWcaaqa aiabgkGi2cqaaiabgkGi2kaadQfaaaWaamWaaeaadaWcaaqaaiabgk Gi2oaaCaaaleqabaGaaGOmaaaaaOqaaiabgkGi2kaadQfadaahaaWc beqaaiaaikdaaaaaaOGaey4kaSIaamOuamaabmaabaWaaSaaaeaacq GHciITdaahaaWcbeqaaiaaikdaaaaakeaacqGHciITcaWGybWaaWba aSqabeaacaaIYaaaaaaakiabgUcaRmaalaaabaGaeyOaIy7aaWbaaS qabeaacaaIYaaaaaGcbaGaeyOaIyRaamywamaaCaaaleqabaGaaGOm aaaaaaaakiaawIcacaGLPaaaaiaawUfacaGLDbaacqaHgpGAdaahaa WcbeqaaiaaiIcacaaIXaGaaGykaaaakiaabccacaaI9aGaaGimaiaa bccacaqGGaGaaeiiaiaabccacaqGGaGaaeiiaiaabIcacaqGZaGaae inaiaabMcaaaa@63CE@ where, P= ( v p 2 α σ d ) 2 v p       (35) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7caWGqbGaaGypamaalaaabaGaaGikaiaadAhadaqhaaWcbaGaamiC aaqaaiaaikdaaaGccqGHsislcqaHXoqycqaHdpWCdaWgaaWcbaGaam izaaqabaGccaaIPaWaaWbaaSqabeaacaaIYaaaaaGcbaGaamODamaa BaaaleaacaWGWbaabeaaaaGccaqGGaGaaeiiaiaabccacaqGGaGaae iiaiaabccacaqGOaGaae4maiaabwdacaqGPaaaaa@4E23@ Q= 1 2 [ μ i ( μ e μ p )( 2γ β 2 ) ]      (36) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7caGGTbGaai4BaiaacsgacaaIXaGaamyBaiaad2gacaWGrbGaaGyp amaalaaabaGaaGymaaqaaiaaikdaaaWaamWaaeaacqaH8oqBdaWgaa WcbaGaamyAaaqabaGccqGHsislcaaIOaGaeqiVd02aaSbaaSqaaiaa dwgaaeqaaOGaeyOeI0IaeqiVd02aaSbaaSqaaiaadchaaeqaaOGaaG ykaiaaiIcadaWcaaqaaiaaikdacqGHsislcqaHZoWzaeaacqaHYoGy daahaaWcbeqaaiaaikdaaaaaaOGaaGykaaGaay5waiaaw2faaiaabc cacaqGGaGaaeiiaiaabccacaqGGaGaaeiiaiaabIcacaqGZaGaaeOn aiaabMcaaaa@5D53@ R=1+ v p 4 ω cd 2 ( v p 2 α σ d ) 2       (37) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7caWGsbGaaGypaiaaigdacqGHRaWkdaWcaaqaaiaadAhadaqhaaWc baGaamiCaaqaaiaaisdaaaaakeaacqaHjpWDdaqhaaWcbaGaam4yai aadsgaaeaacaaIYaaaaOGaaGikaiaadAhadaqhaaWcbaGaamiCaaqa aiaaikdaaaGccqGHsislcqaHXoqycqaHdpWCdaWgaaWcbaGaamizaa qabaGccaaIPaWaaWbaaSqabeaacaaIYaaaaaaakiaabccacaqGGaGa aeiiaiaabccacaqGGaGaaeiiaiaabIcacaqGZaGaae4naiaabMcaaa a@5514@ Equation (34) is a ZK equation for adiabatic DASW’s with Maxwellian ions, degenerate electrons and positrons.
Figure 8: P=0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiuaiaai2 dacaaIWaaaaa@384B@ graph, showing the variation of β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdigaaa@3796@ with μ e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaaaa@38C1@ and μ p MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadchaaeqaaaaa@38CC@ for the values of α=0.5,  μ i =0.4 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGynaiaacYcacaqGGaGaeqiVd02aaSbaaSqa aiaadMgaaeqaaOGaaGypaiaaicdacaaIUaGaaGinaaaa@41B0@ and γ=5/3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4SdCMaaG ypaiaaiwdacaaIVaGaaG4maaaa@3A98@
Figure 9: P=0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiuaiaai2 dacaaIWaaaaa@384B@ graph, showing the variation of β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdigaaa@3796@ with μ e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaaaa@38C1@ and μ p MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadchaaeqaaaaa@38CC@ for the values of α=0.5,  μ i =0.4 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGynaiaacYcacaqGGaGaeqiVd02aaSbaaSqa aiaadMgaaeqaaOGaaGypaiaaicdacaaIUaGaaGinaaaa@41B0@ and γ=4/3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4SdCMaaG ypaiaaisdacaaIVaGaaG4maaaa@3A97@
Figure 10: Variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for the values of μ p =1,  μ i =0.4,  μ e =1.2, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadchaaeqaaOGaaGypaiaaigdacaGGSaGaaeiiaiabeY7a TnaaBaaaleaacaWGPbaabeaakiaai2dacaaIWaGaaGOlaiaaisdaca GGSaGaaeiiaiabeY7aTnaaBaaaleaacaWGLbaabeaakiaai2dacaaI XaGaaGOlaiaaikdacaGGSaaaaa@494B@ σ d =1,  ω cd =0.3, δ=20   0 , MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4Wdm3aaS baaSqaaiaadsgaaeqaaOGaaGypaiaaigdacaGGSaGaaeiiaiabeM8a 3naaBaaaleaacaWGJbGaamizaaqabaGccaaI9aGaaGimaiaai6caca aIZaGaaiilaiaabccacqaH0oazcaaI9aGaaGOmaiaaicdacaqGGaWa aWbaaSqabeaacaaIWaaaaOGaaiilaaaa@49EF@ β=0.7,  u 0 =0.1, α=0.3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaicdacaaIUaGaaG4naiaacYcacaqGGaGaamyDamaaBaaaleaa caaIWaaabeaakiaai2dacaaIWaGaaGOlaiaaigdacaGGSaGaaeiiai abeg7aHjaai2dacaaIWaGaaGOlaiaaiodaaaa@46A9@ (Red), α=0.4 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGinaaaa@3A8B@ (Blue) and α=0.5 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGynaaaa@3A8C@ (Black). Here dotted curve represented ultra-relativistic (γ=4/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI0aGaaG4laiaaiodacaGGPaaaaa@3BF0@ case and solid curve represented non-relativistic (γ=5/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI1aGaaG4laiaaiodacaGGPaaaaa@3BF1@
Figure 11: Variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for the values of α=0.5, β=0.7,  u 0 =0.1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGynaiaacYcacaqGGaGaeqOSdiMaaGypaiaa icdacaaIUaGaaG4naiaacYcacaqGGaGaamyDamaaBaaaleaacaaIWa aabeaakiaai2dacaaIWaGaaGOlaiaaigdaaaa@46AB@ μ p =1,  ω cd =0.3, δ=20   0 , MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadchaaeqaaOGaaGypaiaaigdacaGGSaGaaeiiaiabeM8a 3naaBaaaleaacaWGJbGaamizaaqabaGccaaI9aGaaGimaiaai6caca aIZaGaaiilaiaabccacqaH0oazcaaI9aGaaGOmaiaaicdacaqGGaWa aWbaaSqabeaacaaIWaaaaaaa@4934@ μ e =1.2,  σ d =1,  μ i =0.4 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaOGaaGypaiaaigdacaaIUaGaaGOmaiaacYca caqGGaGaeq4Wdm3aaSbaaSqaaiaadsgaaeqaaOGaaGypaiaaigdaca GGSaGaaeiiaiabeY7aTnaaBaaaleaacaWGPbaabeaakiaai2dacaaI WaGaaGOlaiaaisdaaaa@489C@ (Black), μ i =0.5 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadMgaaeqaaOGaaGypaiaaicdacaaIUaGaaGynaaaa@3BC7@ (Blue) and μ i =0.6 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadMgaaeqaaOGaaGypaiaaicdacaaIUaGaaGOnaaaa@3BC8@ (Red). Here dotted curve represented ultra-relativistic (γ=4/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI0aGaaG4laiaaiodacaGGPaaaaa@3BF0@ case and solid curve represented non-relativistic (γ=5/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI1aGaaG4laiaaiodacaGGPaaaaa@3BF1@ case.
Solution of Zakharov-Kuznetsov Equation
The stationary solution (for simplicity, we have write φ (1) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdO2aaW baaSqabeaacaaIOaGaaGymaiaaiMcaaaaaaa@39FF@ as φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ ) of this ZK equation as,
φ(ξ)= φ m sec h 2 (kξ)     (38) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7cqaHgpGAcaaIOaGaeqOVdGNaaGykaiaai2dacqaHgpGAdaWgaaWc baGaamyBaaqabaGccaWGZbGaamyzaiaadogacaWGObWaaWbaaSqabe aacaaIYaaaaOGaaGikaiaadUgacqaH+oaEcaaIPaGaaeiiaiaabcca caqGGaGaaeiiaiaabccacaqGOaGaae4maiaabIdacaqGPaaaaa@505B@
where φ m =[ 3 u 0 δ 1 ] MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdO2aaS baaSqaaiaad2gaaeqaaOGaaGypaiaaiUfadaWcaaqaaiaaiodacaWG 1bWaaSbaaSqaaiaaicdaaeqaaaGcbaGaeqiTdq2aaSbaaSqaaiaaig daaeqaaaaakiaai2faaaa@40BA@ is the amplitude and k= u 0 4 δ 2 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4Aaiaai2 dadaGcaaqaamaalaaabaGaamyDamaaBaaaleaacaaIWaaabeaaaOqa aiaaisdacqaH0oazdaWgaaWcbaGaaGOmaaqabaaaaaqabaaaaa@3D01@ is the inverse of the width ( Δ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeuiLdqeaaa@375B@ ) of the SW’s respectively; with δ 1 =PQcosδ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiTdq2aaS baaSqaaiaaigdaaeqaaOGaaGypaiaadcfacaWGrbGaai4yaiaac+ga caGGZbGaeqiTdqgaaa@3F73@ and δ 2 = 1 2 P( cos 3 δ+R sin 2 δcosδ), δ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiTdq2aaS baaSqaaiaaikdaaeqaaOGaaGypamaalaaabaGaaGymaaqaaiaaikda aaGaamiuaiaaiIcadaqfGaqabSqabeaacaaIZaaakeaacaGGJbGaai 4BaiaacohaaaGaeqiTdqMaey4kaSIaamOuamaavacabeWcbeqaaiaa ikdaaOqaaiaacohacaGGPbGaaiOBaaaacqaH0oazcaGGJbGaai4Bai aacohacqaH0oazcaaIPaGaaiilaiaabccacqaH0oazaaa@514B@ being the propagation angle of SW’s.

The A=0(P=0) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyqaiaai2 dacaaIWaGaaGikaiaadcfacaaI9aGaaGimaiaaiMcaaaa@3BF7@ surface plots are shown for non-relativistic and ultra-relativistic case in absence (presence) of magnetic field are shown in figure 1 and 2 (8 and 9) respectively. From these figures we find that the SW’s have positive potentials above the surface and negative potentials below the surface. Figure 3 shows the variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for ultra-relativistic and non-relativistic cases. Figure 4, 5, 6 and 7 showing the variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ respectively for the different value of α,  σ d , β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaai ilaiaabccacqaHdpWCdaWgaaWcbaGaamizaaqabaGccaGGSaGaaeii aiabek7aIbaa@3EBD@ and μ p MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadchaaeqaaaaa@38CC@ . All of these figure shows the variation of amplitude and width for ultrarelativistic and non-relativistic cases in the absence of magnetic field. Figure 10, 11, 12, 13, 14 and 15 showing the variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for the value of α,  μ i , δ,  μ e ,  σ d MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaai ilaiaabccacqaH8oqBdaWgaaWcbaGaamyAaaqabaGccaGGSaGaaeii aiabes7aKjaacYcacaqGGaGaeqiVd02aaSbaaSqaaiaadwgaaeqaaO GaaiilaiaabccacqaHdpWCdaWgaaWcbaGaamizaaqabaaaaa@470D@ and β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdigaaa@3796@ respectively in the presence of magnetic field.
Figure 12: Variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for the values of β=0.7, α=0.5,  u 0 =0.1, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbiqaaawfcqaHYo GycaaI9aGaaGimaiaai6cacaaI3aGaaiilaiaabccacqaHXoqycaaI 9aGaaGimaiaai6cacaaI1aGaaiilaiaabccacaWG1bWaaSbaaSqaai aaicdaaeqaaOGaaGypaiaaicdacaaIUaGaaGymaiaacYcaaaa@47D3@ μ p =1,  μ i =0.4,  μ e =1.2, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadchaaeqaaOGaaGypaiaaigdacaGGSaGaaeiiaiabeY7a TnaaBaaaleaacaWGPbaabeaakiaai2dacaaIWaGaaGOlaiaaisdaca GGSaGaaeiiaiabeY7aTnaaBaaaleaacaWGLbaabeaakiaai2dacaaI XaGaaGOlaiaaikdacaGGSaaaaa@494B@ σ d =1,  ω cd =0.3, δ=20   0 , MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4Wdm3aaS baaSqaaiaadsgaaeqaaOGaaGypaiaaigdacaGGSaGaaeiiaiabeM8a 3naaBaaaleaacaWGJbGaamizaaqabaGccaaI9aGaaGimaiaai6caca aIZaGaaiilaiaabccacqaH0oazcaaI9aGaaGOmaiaaicdacaqGGaWa aWbaaSqabeaacaaIWaaaaOGaaiilaaaa@49EF@ (Red), δ=30   0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiTdqMaaG ypaiaaiodacaaIWaGaaeiiamaaCaaaleqabaGaaGimaaaaaaa@3B62@ (Blue) and δ=40   0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiTdqMaaG ypaiaaisdacaaIWaGaaeiiamaaCaaaleqabaGaaGimaaaaaaa@3B63@ (Black). Here dotted curve represented ultra-relativistic (γ=4/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI0aGaaG4laiaaiodacaGGPaaaaa@3BF0@ case and solid curve represented non-relativistic (γ=5/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI1aGaaG4laiaaiodacaGGPaaaaa@3BF1@ case.
Instability
We now study the instability of the opaquely propagating solitary waves, discussed in the previous section, by the method of small- perturbation expansion (22-28). We first assume that separate φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ as a function of ψ 0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiYdK3aaS baaSqaaiaaicdaaeqaaaaa@38A9@ and ψ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiYdKhaaa@37C3@ as
φ= ψ 0 (Z)+ψ(ξ,ζ,η,t)      (39) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7cqaHgpGAcaaI9aGaeqiYdK3aaSbaaSqaaiaaicdaaeqaaOGaaGik aiaadQfacaaIPaGaey4kaSIaeqiYdKNaaGikaiabe67a4jaaiYcacq aH2oGEcaaISaGaeq4TdGMaaGilaiaadshacaaIPaGaaeiiaiaabcca caqGGaGaaeiiaiaabccacaqGGaGaaeikaiaabodacaqG5aGaaeykaa aa@538E@
Where ξ, ζ, η MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGNaai ilaiaabccacqaH2oGEcaGGSaGaaeiiaiabeE7aObaa@3DC7@ and t MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiDaaaa@36EE@ are components of new reference frame. For a long-wavelength plane wave perturbation in a direction with direction cosines ( l ζ , l η , l ξ ), ψ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGikaiaadY gadaWgaaWcbaGaeqOTdOhabeaakiaaiYcacaWGSbWaaSbaaSqaaiab eE7aObqabaGccaaISaGaamiBamaaBaaaleaacqaH+oaEaeqaaOGaaG ykaiaacYcacaqGGaGaeqiYdKhaaa@4488@ is given by
ψ=ϕ(Z) e i[k( l ζ ζ+ l η η+ l ξ Z)ωt]      (40) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7cqaHipqEcaaI9aGaeqy1dyMaaGikaiaadQfacaaIPaGaamyzamaa CaaaleqabaGaamyAaiaaiUfacaWGRbGaaGikaiaadYgadaWgaaqaai abeA7a6bqabaGccqaH2oGEcqGHRaWkcaWGSbWaaSbaaSqaaiabeE7a ObqabaGccqaH3oaAcqGHRaWkcaWGSbWaaSbaaSqaaiabe67a4bqaba GccaWGAbGaaGykaiabgkHiTiabeM8a3jaadshacaaIDbaaaiaabcca caqGGaGaaeiiaiaabccacaqGGaGaaeikaiaabsdacaqGWaGaaeykaa aa@5E1D@
in which l ζ 2 + l η 2 + l ξ 2 =1, k MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiBamaaDa aaleaacqaH2oGEaeaacaaIYaaaaOGaey4kaSIaamiBamaaDaaaleaa cqaH3oaAaeaacaaIYaaaaOGaey4kaSIaamiBamaaDaaaleaacqaH+o aEaeaacaaIYaaaaOGaaGypaiaaigdacaGGSaGaaeiiaiaadUgaaaa@4656@ is the wave constant, ω MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdChaaa@37C2@ is the angular frequency of the waves and ϕ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqy1dygaaa@37BD@ is the amplitude of the waves.

For small k, ϕ(Z) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiaacY cacaqGGaGaeqy1dyMaaGikaiaadQfacaaIPaaaaa@3C44@ and ω MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdChaaa@37C2@ can be expanded as ϕ(Z)= ϕ 0 (Z)+k ϕ 1 (Z)+ k 2 ϕ 2 (Z)+     (41) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7cqaHvpGzcaaIOaGaamOwaiaaiMcacaaI9aGaeqy1dy2aaSbaaSqa aiaaicdaaeqaaOGaaGikaiaadQfacaaIPaGaey4kaSIaam4Aaiabew 9aMnaaBaaaleaacaaIXaaabeaakiaaiIcacaWGAbGaaGykaiabgUca RiaadUgadaahaaWcbeqaaiaaikdaaaGccqaHvpGzdaWgaaWcbaGaaG OmaaqabaGccaaIOaGaamOwaiaaiMcacqGHRaWkcqGHflY1cqGHflY1 cqGHflY1caqGGaGaaeiiaiaabccacaqGGaGaaeiiaiaabIcacaqG0a GaaeymaiaabMcaaaa@5F23@ ω=k ω 1 + k 2 ω 2 +      (42) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7cqaHjpWDcaaI9aGaam4AaiabeM8a3naaBaaaleaacaaIXaaabeaa kiabgUcaRiaadUgadaahaaWcbeqaaiaaikdaaaGccqaHjpWDdaWgaa WcbaGaaGOmaaqabaGccqGHRaWkcqGHflY1cqGHflY1cqGHflY1caqG GaGaaeiiaiaabccacaqGGaGaaeiiaiaabccacaqGOaGaaeinaiaabk dacaqGPaaaaa@532C@ Doing some mathematical analysis we arrive at the following dispersion relation:
Figure 13: Variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for the values of β=0.7,  σ d =1,  u 0 =0.1, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaicdacaaIUaGaaG4naiaacYcacaqGGaGaeq4Wdm3aaSbaaSqa aiaadsgaaeqaaOGaaGypaiaaigdacaGGSaGaaeiiaiaadwhadaWgaa WcbaGaaGimaaqabaGccaaI9aGaaGimaiaai6cacaaIXaGaaiilaaaa @4728@ ω cd =0.3, δ=20   0 , α=0.5 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdC3aaS baaSqaaiaadogacaWGKbaabeaakiaai2dacaaIWaGaaGOlaiaaioda caGGSaGaaeiiaiabes7aKjaai2dacaaIYaGaaGimaiaabccadaahaa WcbeqaaiaaicdaaaGccaGGSaGaaeiiaiabeg7aHjaai2dacaaIWaGa aGOlaiaaiwdaaaa@4972@ μ p =1, μ i =0.4,  μ e =1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadchaaeqaaOGaaGypaiaaigdacaGGSaGaaGPaVlabeY7a TnaaBaaaleaacaWGPbaabeaakiaai2dacaaIWaGaaGOlaiaaisdaca GGSaGaaeiiaiabeY7aTnaaBaaaleaacaWGLbaabeaakiaai2dacaaI Xaaaaa@480F@ (Red), μ e =1.1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaOGaaGypaiaaigdacaaIUaGaaGymaaaa@3BC0@ (Blue) and μ e =1.2 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaOGaaGypaiaaigdacaaIUaGaaGOmaaaa@3BC1@ (Black). Here dotted curve represented ultra-relativistic (γ=4/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI0aGaaG4laiaaiodacaGGPaaaaa@3BF0@ case and solid curve represented non-relativistic (γ=5/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI1aGaaG4laiaaiodacaGGPaaaaa@3BF1@ case.
Figure 14: Variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for the values of β=0.7,  ω cd =0.3, δ=20 0 , MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaicdacaaIUaGaaG4naiaacYcacaqGGaGaeqyYdC3aaSbaaSqa aiaadogacaWGKbaabeaakiaai2dacaaIWaGaaGOlaiaaiodacaGGSa Gaaeiiaiabes7aKjaai2dacaaIYaGaaGimaiaaykW7daahaaWcbeqa aiaaicdaaaGccaGGSaaaaa@4B0E@ α=0.5,  u 0 =0.1,  μ p =1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGynaiaacYcacaqGGaGaamyDamaaBaaaleaa caaIWaaabeaakiaai2dacaaIWaGaaGOlaiaaigdacaGGSaGaaeiiai abeY7aTnaaBaaaleaacaWGWbaabeaakiaai2dacaaIXaaaaa@4673@ μ i =0.4, μ e =1.2,  σ d =0.6 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadMgaaeqaaOGaaGypaiaaicdacaaIUaGaaGinaiaacYca caaMc8UaeqiVd02aaSbaaSqaaiaadwgaaeqaaOGaaGypaiaaigdaca aIUaGaaGOmaiaacYcacaqGGaGaeq4Wdm3aaSbaaSqaaiaadsgaaeqa aOGaaGypaiaaicdacaaIUaGaaGOnaaaa@4AFB@ (Red), σ d =0.8 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4Wdm3aaS baaSqaaiaadsgaaeqaaOGaaGypaiaaicdacaaIUaGaaGioaaaa@3BD2@ (Blue) and σ d =1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4Wdm3aaS baaSqaaiaadsgaaeqaaOGaaGypaiaaigdaaaa@3A59@ (Black). Here dotted curve represented ultra-relativistic (γ=4/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI0aGaaG4laiaaiodacaGGPaaaaa@3BF0@ case and solid curve represented non-relativistic (γ=5/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI1aGaaG4laiaaiodacaGGPaaaaa@3BF1@ case.
ω 1 =Ω l ξ U 0 +( Ω 2 ϒ)   1/2       (43) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7cqaHjpWDdaWgaaWcbaGaaGymaaqabaGccaaI9aGaeuyQdCLaeyOe I0IaamiBamaaBaaaleaacqaH+oaEaeqaaOGaamyvamaaBaaaleaaca aIWaaabeaakiabgUcaRiaaiIcacqqHPoWvdaahaaWcbeqaaiaaikda aaGccqGHsislcqqHspqOcaaIPaGaaeiiamaaCaaaleqabaGaaGymai aai+cacaaIYaaaaOGaaeiiaiaabccacaqGGaGaaeiiaiaabccacaqG GaGaaeikaiaabsdacaqGZaGaaeykaaaa@551B@
where Ω= 2 3 ( ψ m μ 1 2 μ 2 κ 2 ) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7caGGTbGaai4BaiaacsgacaaIQaGaeyOeI0IaaGymaiaadogacaWG TbGaeuyQdCLaaGypamaalaaabaGaaGOmaaqaaiaaiodaaaGaaGikai abeI8a5naaBaaaleaacaWGTbaabeaakiabeY7aTnaaBaaaleaacaaI XaaabeaakiabgkHiTiaaikdacqaH8oqBdaWgaaWcbaGaaGOmaaqaba GccqaH6oWAdaahaaWcbeqaaiaaikdaaaGccaaIPaaaaa@51E9@ ϒ= 16 45 ( ψ m 2 μ 1 2 3 ψ m μ 1 μ 2 κ 2 3 μ 2 2 κ 4 +12 δ 2 μ 3 κ 4 ) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7caGGTbGaai4BaiaacsgacaaIQaGaeyOeI0IaaGymaiaadogacaWG TbGaeuO0deQaaGypamaalaaabaGaaGymaiaaiAdaaeaacaaI0aGaaG ynaaaacaaIOaGaeqiYdK3aa0baaSqaaiaad2gaaeaacaaIYaaaaOGa eqiVd02aa0baaSqaaiaaigdaaeaacaaIYaaaaOGaeyOeI0IaaG4mai abeI8a5naaBaaaleaacaWGTbaabeaakiabeY7aTnaaBaaaleaacaaI XaaabeaakiabeY7aTnaaBaaaleaacaaIYaaabeaakiabeQ7aRnaaCa aaleqabaGaaGOmaaaakiabgkHiTiaaiodacqaH8oqBdaqhaaWcbaGa aGOmaaqaaiaaikdaaaGccqaH6oWAdaahaaWcbeqaaiaaisdaaaGccq GHRaWkcaaIXaGaaGOmaiabes7aKnaaBaaaleaacaaIYaaabeaakiab eY7aTnaaBaaaleaacaaIZaaabeaakiabeQ7aRnaaCaaaleqabaGaaG inaaaakiaaiMcaaaa@6CE9@ with, μ 1 = δ 1 l ξ + δ 3 l ζ μ 2 =3 δ 2 l ξ + δ 5 l ζ μ 3 =3 δ 2 l ξ 2 +2 δ 5 l ζ l ξ + δ 6 l ζ 2 + δ 7 l η 2 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGceaqabeaacaaMf8 UaaGzbVlabeY7aTnaaBaaaleaacaaIXaaabeaakiaai2dacqaH0oaz daWgaaWcbaGaaGymaaqabaGccaWGSbWaaSbaaSqaaiabe67a4bqaba GccqGHRaWkcqaH0oazdaWgaaWcbaGaaG4maaqabaGccaWGSbWaaSba aSqaaiabeA7a6bqabaaakeaacaaMf8UaaGzbVlabeY7aTnaaBaaale aacaaIYaaabeaakiaai2dacaaIZaGaeqiTdq2aaSbaaSqaaiaaikda aeqaaOGaamiBamaaBaaaleaacqaH+oaEaeqaaOGaey4kaSIaeqiTdq 2aaSbaaSqaaiaaiwdaaeqaaOGaamiBamaaBaaaleaacqaH2oGEaeqa aaGcbaGaaGzbVlaaywW7cqaH8oqBdaWgaaWcbaGaaG4maaqabaGcca aI9aGaaG4maiabes7aKnaaBaaaleaacaaIYaaabeaakiaadYgadaqh aaWcbaGaeqOVdGhabaGaaGOmaaaakiabgUcaRiaaikdacqaH0oazda WgaaWcbaGaaGynaaqabaGccaWGSbWaaSbaaSqaaiabeA7a6bqabaGc caWGSbWaaSbaaSqaaiabe67a4bqabaGccqGHRaWkcqaH0oazdaWgaa WcbaGaaGOnaaqabaGccaWGSbWaa0baaSqaaiabeA7a6bqaaiaaikda aaGccqGHRaWkcqaH0oazdaWgaaWcbaGaaG4naaqabaGccaWGSbWaa0 baaSqaaiabeE7aObqaaiaaikdaaaaaaaa@813D@ It is clear from the dispersion relation (43) that there is always instability if (ϒ Ω 2 )>0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGikaiabfk 9aHkabgkHiTiabfM6axnaaCaaaleqabaGaaGOmaaaakiaaiMcacaaI +aGaaGimaaaa@3E4B@ We can express the instability criterion as S i >0     (44) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7caWGtbWaaSbaaSqaaiaadMgaaeqaaOGaaGOpaiaaicdacaqGGaGa aeiiaiaabccacaqGGaGaaeiiaiaabIcacaqG0aGaaeinaiaabMcaaa a@4283@ with S i = l η 2 [ ω cd 2 + sin 2 δ]+ l ζ 2 [ ω cd 2 5 3 ( ω cd 2 +1) tan 2 δ ]    (45) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7caGGTbGaai4BaiaacsgacaaIQaGaeyOeI0IaaGymaiaadogacaWG TbGaam4uamaaBaaaleaacaWGPbaabeaakiaai2dacaWGSbWaa0baaS qaaiabeE7aObqaaiaaikdaaaGccaaIBbGaeqyYdC3aa0baaSqaaiaa dogacaWGKbaabaGaaGOmaaaakiabgUcaRmaavacabeWcbeqaaiaaik daaOqaaiaacohacaGGPbGaaiOBaaaacqaH0oazcaaIDbGaey4kaSIa amiBamaaDaaaleaacqaH2oGEaeaacaaIYaaaaOWaamWaaeaacqaHjp WDdaqhaaWcbaGaam4yaiaadsgaaeaacaaIYaaaaOGaeyOeI0YaaSaa aeaacaaI1aaabaGaaG4maaaacaaIOaGaeqyYdC3aa0baaSqaaiaado gacaWGKbaabaGaaGOmaaaakiabgUcaRiaaigdacaaIPaWaaubiaeqa leqabaGaaGOmaaGcbaGaaiiDaiaacggacaGGUbaaaiabes7aKbGaay 5waiaaw2faaiaabccacaqGGaGaaeiiaiaabccacaqGOaGaaeinaiaa bwdacaqGPaaaaa@7316@ If this instability criterion S i >0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4uamaaBa aaleaacaWGPbaabeaakiaai6dacaaIWaaaaa@3973@ is satisfied, the growth rate Γ=(ϒ Ω 2 )   1/2 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeu4KdCKaey ypa0Jaaiikaiabfk9aHkabgkHiTiabfM6axnaaCaaaleqabaGaaGOm aaaakiaacMcacaqGGaWaaWbaaSqabeaacaaIXaGaai4laiaaikdaaa aaaa@4225@ of the unstable perturbation of these solitary waves is given by
Figure 15: Variation of φ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B2@ with ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOVdGhaaa@37B8@ for the values of α=0.5,  ω cd =0.3, δ=20   0 , MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGynaiaacYcacaqGGaGaeqyYdC3aaSbaaSqa aiaadogacaWGKbaabeaakiaai2dacaaIWaGaaGOlaiaaiodacaGGSa Gaaeiiaiabes7aKjaai2dacaaIYaGaaGimaiaabccadaahaaWcbeqa aiaaicdaaaGccaGGSaaaaa@4A22@ u 0 =0.1, μ p =1,  μ i =0.4, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyDamaaBa aaleaacaaIWaaabeaakiaai2dacaaIWaGaaGOlaiaaigdacaGGSaGa aGPaVlabeY7aTnaaBaaaleaacaWGWbaabeaakiaai2dacaaIXaGaai ilaiaabccacqaH8oqBdaWgaaWcbaGaamyAaaqabaGccaaI9aGaaGim aiaai6cacaaI0aGaaiilaaaa@4945@ μ e =1.2,  σ d =1, β=0.6 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaOGaaGypaiaaigdacaaIUaGaaGOmaiaacYca caqGGaGaeq4Wdm3aaSbaaSqaaiaadsgaaeqaaOGaaGypaiaaigdaca GGSaGaaeiiaiabek7aIjaai2dacaaIWaGaaGOlaiaaiAdaaaa@4765@ (Black), β=0.7 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaicdacaaIUaGaaG4naaaa@3A90@ (Blue) and β=0.8 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaicdacaaIUaGaaGioaaaa@3A91@ (Red). Here dotted curve represented ultra-relativistic (γ=4/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI0aGaaG4laiaaiodacaGGPaaaaa@3BF0@ case and solid curve represented non-relativistic (γ=5/3) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiabeo 7aNjaai2dacaaI1aGaaG4laiaaiodacaGGPaaaaa@3BF1@ case.
Figure 16: S i =0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4uamaaBa aaleaacaWGPbaabeaakiaai2dacaaIWaaaaa@3972@ surface plot showing the variation of ω cd MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdC3aaS baaSqaaiaadogacaWGKbaabeaaaaa@39BF@ with l η MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiBamaaBa aaleaacqaH3oaAaeqaaaaa@38BE@ and l ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiBamaaBa aaleaacqaH+oaEaeqaaaaa@38D5@ for the values of μ e =1.2,  μ p =1,  μ i =0.4, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaOGaaGypaiaaigdacaaIUaGaaGOmaiaacYca caqGGaGaeqiVd02aaSbaaSqaaiaadchaaeqaaOGaaGypaiaaigdaca GGSaGaaeiiaiabeY7aTnaaBaaaleaacaWGPbaabeaakiaai2dacaaI WaGaaGOlaiaaisdacaGGSaaaaa@494B@ β=1,  α=0.5, σ=1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaigdacaGGSaGaaeiiaiabeg7aHjaai2dacaaIWaGaaGOlaiaa iwdacaGGSaGaaeiiaiabeo8aZjaai2dacaaIXaaaaa@439A@ and δ=20   0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiTdqMaaG ypaiaaikdacaaIWaGaaeiiamaaCaaaleqabaGaaGimaaaaaaa@3B61@ .
Γ= 2 15 U 0 ( ω cd 2 + sin 2 δ)   ( ω cd 2 +1) S i        (46) MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGzbVlaayw W7cqqHtoWrcaaI9aWaaSaaaeaacaaIYaaabaWaaOaaaeaacaaIXaGa aGynaaWcbeaaaaGcdaWcaaqaaiaadwfadaWgaaWcbaGaaGimaaqaba aakeaacaaIOaGaeqyYdC3aa0baaSqaaiaadogacaWGKbaabaGaaGOm aaaakiabgUcaRmaavacabeWcbeqaaiaaikdaaOqaaiaacohacaGGPb GaaiOBaaaacqaH0oazcaaIPaaaaiaabccadaGcaaqaaiaaiIcacqaH jpWDdaqhaaWcbaGaam4yaiaadsgaaeaacaaIYaaaaOGaey4kaSIaaG ymaiaaiMcacaWGtbWaaSbaaSqaaiaadMgaaeqaaaqabaGccaqGGaGa aeiiaiaabccacaqGGaGaaeiiaiaabccacaqGGaGaaeikaiaabsdaca qG2aGaaeykaaaa@5D65@
Figure 16 represent S i =0 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4uamaaBa aaleaacaWGPbaabeaakiaai2dacaaIWaaaaa@3972@ surface plot showing the variation of ω cd MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdC3aaS baaSqaaiaadogacaWGKbaabeaaaaa@39BF@ with l η MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiBamaaBa aaleaacqaH3oaAaeqaaaaa@38BE@ and l ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiBamaaBa aaleaacqaH+oaEaeqaaaaa@38D5@ , From this figure we found that ω cd MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdC3aaS baaSqaaiaadogacaWGKbaabeaaaaa@39BF@ decreases with increasing the value of l η MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiBamaaBa aaleaacqaH3oaAaeqaaaaa@38BE@ very rapidly and increases slowly with increasing the value of l ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiBamaaBa aaleaacqaH+oaEaeqaaaaa@38D5@ Figure 17 showing the variation of growth rate Γ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeu4KdCeaaa@375D@ with σ d MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4Wdm3aaS baaSqaaiaadsgaaeqaaaaa@38CD@ and β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdigaaa@3796@ We found from this figure that Γ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeu4KdCeaaa@375D@ decreases with increasing the value of σ d MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4Wdm3aaS baaSqaaiaadsgaaeqaaaaa@38CD@ and β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdigaaa@3796@ Figure 18 shows the variation of Γ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeu4KdCeaaa@375D@ with μ i MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadMgaaeqaaaaa@38C5@ and μ e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaaaa@38C1@ We have found from this figure that Γ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeu4KdCeaaa@375D@ decreases with increasing the value of μ e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaaaa@38C1@ and μ i MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadMgaaeqaaaaa@38C5@ Figure 19 has shown the variation of growth rate Γ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeu4KdCeaaa@375D@ with α MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdegaaa@3794@ and β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdigaaa@3796@ We have seen from the figure that Γ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeu4KdCeaaa@375D@ increases with increasing the value of α MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdegaaa@3794@ .
Findings
DA SW’s have been examined in a collisionless dusty plasma consisting of inertialess ultra-relativistic and non-relativistic electrons and positrons, inertial mobile positive dust particles, inertial Maxwellian ions by deriving K-dV equation using reductive perturbation technique. It has been found that the basic features of such DA solitary waves are significantly modified by the presence degeneracy of adiabaticness of components. The effects of the parametric regimes on solitary wave for both case of unmagnetic and magnetic fields are discussed below:

1. Depending on the value of μ e ,  μ p MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaOGaaiilaiaabccacqaH8oqBdaWgaaWcbaGa amiCaaqabaaaaa@3CF5@ and β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdigaaa@3796@ the solitary waves can be associated with positive (negative) potentials above (below) the A = 0 surface for unmagnetized and P = 0 surface for magnetized plasmas respectively.

2. The amplitude of the DASW’s is higher for ultrarelativistic case than non-relativistic one.

3. Magnetic field enhance the amplitude of the SW’s for both ultra-relativistic and non-relativistic case.

4. Both amplitude and width of the solitary waves increases with increasing the value of α, δ,  σ d MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaai ilaiaabccacqaH0oazcaGGSaGaaeiiaiabeo8aZnaaBaaaleaacaWG Kbaabeaaaaa@3EB7@ μ e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaaaa@38C1@ but decreases with increasing the value of μ i ,  μ p MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadMgaaeqaaOGaaiilaiaabccacqaH8oqBdaWgaaWcbaGa amiCaaqabaaaaa@3CF9@ and β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdigaaa@3796@ in the case of unmagnetized as well as magnetized dusty plasmas.

5. Cyclotron frequency ω cd MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdC3aaS baaSqaaiaadogacaWGKbaabeaaaaa@39BF@ increases with increasing the value of l η MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiBamaaBa aaleaacqaH3oaAaeqaaaaa@38BE@ and decreasing the value of l ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiBamaaBa aaleaacqaH+oaEaeqaaaaa@38D5@ .

6. The growth rate Γ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeu4KdCeaaa@375D@ ecreases with increasing the value of σ, β,  μ e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4WdmNaai ilaiaabccacqaHYoGycaGGSaGaaeiiaiabeY7aTnaaBaaaleaacaWG Lbaabeaaaaa@3ECB@ and μ i MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadMgaaeqaaaaa@38C5@ but increases with increasing the value of α MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdegaaa@3794@ .
Figure 17: Variation of growth rate ( Γ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeu4KdCeaaa@375D@ ) with σ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4Wdmhaaa@37B8@ and β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdigaaa@3796@ for the values of μ e =1.2,  μ p =1,  μ i =0.4, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaOGaaGypaiaaigdacaaIUaGaaGOmaiaacYca caaMc8UaaeiiaiabeY7aTnaaBaaaleaacaWGWbaabeaakiaai2daca aIXaGaaiilaiaabccacqaH8oqBdaWgaaWcbaGaamyAaaqabaGccaaI 9aGaaGimaiaai6cacaaI0aGaaiilaaaa@4AD6@ δ=2   0 , α=0.2,  l η =0.4, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiTdqMaaG ypaiaaikdacaqGGaWaaWbaaSqabeaacaaIWaaaaOGaaiilaiaabcca cqaHXoqycaaI9aGaaGimaiaai6cacaaIYaGaaiilaiaaykW7caqGGa GaamiBamaaBaaaleaacqaH3oaAaeqaaOGaaGypaiaaicdacaaIUaGa aGinaiaacYcaaaa@49F0@ l ξ =0.5,  u 0 =0.1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiBamaaBa aaleaacqaH+oaEaeqaaOGaaGypaiaaicdacaaIUaGaaGynaiaacYca caqGGaGaamyDamaaBaaaleaacaaIWaaabeaakiaai2dacaaIWaGaaG Olaiaaigdaaaa@4208@ and ω cd =0.3 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdC3aaS baaSqaaiaadogacaWGKbaabeaakiaai2dacaaIWaGaaGOlaiaaioda aaa@3CBF@ .
Figure 18: Variation of growth rate ( Γ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeu4KdCeaaa@375D@ with μ i MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadMgaaeqaaaaa@38C5@ and μ e MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaaaa@38C1@ for the values of α=0.1, β=0.7,  μ p =1, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaaG ypaiaaicdacaaIUaGaaGymaiaacYcacaqGGaGaeqOSdiMaaGypaiaa icdacaaIUaGaaG4naiaacYcacaqGGaGaeqiVd02aaSbaaSqaaiaadc haaeqaaOGaaGypaiaaigdacaGGSaaaaa@46DC@ ω cd =0.5,  l ξ =0.5,  l η =0.4, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdC3aaS baaSqaaiaadogacaWGKbaabeaakiaai2dacaaIWaGaaGOlaiaaiwda caGGSaGaaeiiaiaadYgadaWgaaWcbaGaeqOVdGhabeaakiaai2daca aIWaGaaGOlaiaaiwdacaGGSaGaaeiiaiaadYgadaWgaaWcbaGaeq4T dGgabeaakiaai2dacaaIWaGaaGOlaiaaisdacaGGSaaaaa@4BC3@ δ=15   0 , σ=1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiTdqMaaG ypaiaaigdacaaI1aGaaeiiamaaCaaaleqabaGaaGimaaaakiaacYca caqGGaGaeq4WdmNaaGypaiaaigdaaaa@4007@ and u 0 =0.1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyDamaaBa aaleaacaaIWaaabeaakiaai2dacaaIWaGaaGOlaiaaigdaaaa@3AD3@ .
Figure 19: Variation of growth rate ( Γ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeu4KdCeaaa@375D@ ) with l η MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiBamaaBa aaleaacqaH3oaAaeqaaaaa@38BE@ and l ξ MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiBamaaBa aaleaacqaH+oaEaeqaaaaa@38D5@ for the values of β=0.7,  μ p =1,  ω cd =0.3, MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaaG ypaiaaicdacaaIUaGaaG4naiaacYcacaaMc8UaaeiiaiabeY7aTnaa BaaaleaacaWGWbaabeaakiaai2dacaaIXaGaaiilaiaabccacqaHjp WDdaWgaaWcbaGaam4yaiaadsgaaeqaaOGaaGypaiaaicdacaaIUaGa aG4maiaacYcaaaa@4A9E@ μ e =1.2,  μ i =0.4, δ=2   0 , MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiVd02aaS baaSqaaiaadwgaaeqaaOGaaGypaiaaigdacaaIUaGaaGOmaiaacYca caqGGaGaeqiVd02aaSbaaSqaaiaadMgaaeqaaOGaaGypaiaaicdaca aIUaGaaGinaiaacYcacaqGGaGaeqiTdqMaaGypaiaaikdacaqGGaWa aWbaaSqabeaacaaIWaaaaOGaaiilaaaa@49A4@ σ=1,  l ξ =0.5 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeq4WdmNaaG ypaiaaigdacaGGSaGaaeiiaiaadYgadaWgaaWcbaGaeqOVdGhabeaa kiaai2dacaaIWaGaaGOlaiaaiwdaaaa@406F@ and u 0 =0.1 MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyDamaaBa aaleaacaaIWaaabeaakiaai2dacaaIWaGaaGOlaiaaigdaaaa@3AD3@ .
Conclusion
In conclusion we can say that Maxwellian ions can modify the basic properties of the solitary waves significantly. On the other hand the presence of magnetic field effects the amplitude and width of the solitary wave and its instability. The properties of the solitary waves also moderated by the presence the adiabetic pressers in degenerate plasmas. We have shown the variation of solitary wave phenomenon and its stabilities criterion as well as its growth rate due to the ultra-relativistic and nonrelativistic degenerate pressure. These theoretical analysis may helpful astrophysicist to understand different critical situations exist in white dwarf and neutron stars; not only that, the other astrophysical objects where degenerate pressure plays a vital role to sustain these. Compering the present analysis to others (non-degenerate objects) one give a prediction on the situation of degenerate astrophysical objects.

The plasma parameters used in the present investigations correspond to white dwarfs though it can also be applied for neutron stars. As the number density of plasma parameters, so as the value of β MathType@MTEF@5@5@+= feaagGart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOSdigaaa@3796@ , is much higher for neutron stars than white dwarfs; it can be predict that the amplitude of the SW’s would be higher. But numerical analysis is essential to view the true fact. We hope we will see the actual variation of wave properties between white dwarf and neutron stars very soon. We hope that our present investigation can helpful for understanding the white dwarfs and neutron stars and give a guideline for then who wants to work in the relevant field.
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