Startseite Effect of Dust Ion Collision on Dust Ion Acoustic Solitary Waves for Nonextensive Plasmas in the Framework of Damped Korteweg–de Vries–Burgers Equation
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Effect of Dust Ion Collision on Dust Ion Acoustic Solitary Waves for Nonextensive Plasmas in the Framework of Damped Korteweg–de Vries–Burgers Equation

  • Niranjan Paul EMAIL logo , Kajal Kumar Mondal und Prasanta Chatterjee
Veröffentlicht/Copyright: 22. Mai 2019

Abstract

Analytical solitary wave solution of the dust ion acoustic waves (DIAWs) is studied in the framework of the damped Korteweg–de Vries–Burgers (DKdVB) equation in an unmagnetised collisional dusty plasma consisting of negatively charged dust grain, positively charged ions, q-nonextensive electrons, and neutral particles. Using Reductive Perturbation Technique, the DKdVB equation is obtained for DIAWs. The effects of different physical parameters such as dust ion collision frequency parameter (νid0), viscosity coefficient (η10), the entropic index (q), the speed of the travelling wave (M0), and the ratio between the unperturbed densities of the electrons and ions (μ) on the analytical solution of DIAWs are observed. The results of the present article may have applications in laboratory and space plasmas.

1 Introduction

From the last three decades, research on dusty plasma is one of the most rapidly growing fields in plasma physics. Nonlinear phenomena like solitons, shock waves, and vortices in dusty plasma have been studied theoretically and experimentally by several researchers [1], [2], [3], [4], [5], [6], [7], [8], [9]. To study nonlinear waves in dusty plasma, several authors have derived Korteweg–de Vries–Burgers (KdVB) equation by Reduction Perturbation Technique (RPT). Sukla and Mamun [10] derived KdVB equation by RPT, and they studied the properties of solitons and shock waves in strongly coupled unmagnetised dusty plasmas. Solitons and shock waves would be the fundamental nonlinear coherent structures in the dusty plasma, and that was studied by Xie et al. [11] and Verheest [12]. In the dusty plasma, it has been observed that if dissipation is weak, then the balance between nonlinear and dispersion effects can form the symmetrical solitary waves, and the strong dissipation effects produce shocks. Dust acoustic solitary structures in the dusty plasma also have been investigated widely by many researchers [13], [14], [15]. Rao et al. [16] observed the shock waves in coupled dusty plasma with Boltzman distribution of ions. There are two types of system depending on the range of the interparticle forces such as extensive system and nonextensive system. The extensive system holds for the system with short-range interparticle forces, and the nonextensive property holds for the system in which long-range interparticle forces (Newtonian gravitational forces and Coulomb electric forces) are present. Roy et al. [17] studied on ion-acoustic shocks in quantum electron–positron–ion plasmas and investigated the nonlinear propagation of quantum ion-acoustic waves in three-component quantum electron–positron–ion plasma. They explained the existence of shock waves and transition of oscillatory to monotonic shocks when either equilibrium electron-to-ion density ratio or kinetic viscosity coefficient exceeds its critical value. Misra et al. [18] showed derivation of KdVB equation with RPT and solved numerically and showed that the perturbations with negative potential may propagate as solitary waves and shocks in plasma with positively charged dusts, whereas solitary waves and shocks with both positive and negative potential may exist when dusts are negatively charged. Das et al. [19] studied the effect of dust ion collision on the dust ion acoustic waves (DIAWs) in the framework of damped Zakharov–Kuznetsov equation. They have shown that the system exhibits quasi-periodic behaviour in absence of dust ion collision and the system became chaotic and when the dust ion collision is taken into consideration. Dev and Deka [20] investigated nonlinear propagation of dust ion acoustic shock waves in dusty pair ion plasma with dust charge fluctuation due to nonthermal positive and negative species in the framework of modified complex Burger equation with complex nonlinear coefficient. Roy et al. [21] studied the effect of ion temperature on ion-acoustic solitary waves in plasma with a q-nonextensive electron velocity distribution. They have shown the existence of compressive solitary waves in two-component plasma using Sagdeep pseudo potential approach. Until today, very few works have been done to study the effect of dust ion collision on DIAWs. However, no work has been reported to show the effects of dust ion collision on DIAWs in the framework of damped Korteweg–de Vries–Burgers (DKdVB) equation. Moreover, until today, no work on analytical solitary wave solution of DKdVB equation is reported.

In this present article, our aim is to derive the analytical solitary wave solution of the DKdVB equation for small values of the coefficients of Burger term and damping term in the dusty plasma for q-nonextensive electrons distribution and to find the effects of the different values of the special parameters such as μ, q, M0, νid0, η10, and τ on the amplitude and the width of the solitary waves.

The remaining part of the article is composed as follows: In Section 2, we have considered the basic equations. Nonlinear analyses are discussed in Section 3. In Section 4, we have obtained numerical simulation for different values of the parameters and present discussion. The conclusions are presented in the Section 5.

2 Basic Equations

In this work, an unmagnetised collisional dusty plasma has been considered that contains cold inertial ions, stationary dusts with negative charge, and q-nonextensive electrons. The normalised ion fluid equations that include the equation of continuity, equation of momentum balance, and Poisson equation, governing the DIAWs, are given by

(1)nt+(nu)x=0,
(2)ut+uux=ϕx+η2ux2νidu,
(3)2ϕx2=(1μ)nen+μ,
(4)ne=ne0{1+(q1)ϕ}q+12(q1)

where n is the number density of ions normalised to its equilibrium value n0, u is the ion fluid velocity normalised to ion acoustic speed Cs=(kBTemi), with Te as electron temperature, kB as Boltzmann constant, and mi as mass of ions. The electrostatic wave potential ϕ is normalised to kBTee, with e as magnitude of electron charge. The space variable x is normalised to the Debye length λD=(Te4πne0e2)12, and time t is normalised to ωpi1=(mi4πne0e2)12, with ωpi as ion–plasma frequency. Here, νid is the dust ion collisional frequency and μ=n0en0i, where n0e and n0i are the unperturbed number densities of electrons and ions, respectively.

In order to describe q-nonextensive electron, we have considered the following distribution function as [22]:

fe(v)=Cq{1+(q1)[mev22kBTeeϕkBTe]}1q1,

where ϕ is the electrostatic potential, and other variables or parameters have their usual meaning. It is highly significant to take that fe(v) as it is the prominent distribution that maximises the Tsallis entropy and keeps the law of thermodynamics. Then, the constant of normalisation is given by

Cq=ne0Γ(11q)Γ(11q12)me(1q)2πkBTe  for1<q<1

and

Cq=ne01+q2Γ(11q+12)Γ(11q)me(1q)2πkBTe  forq>1

Integrating the distribution function fe(v) over the velocity space, one can obtain the q-nonextensive electron number density as

ne=ne0{1+(q1)eϕkBTe}q+12(q1)

Thus, the normalised q-nonextensive electron number density [22] takes the form:

(5)ne=ne0{1+(q1)ϕ}q+12(q1)

3 Nonlinear Analysis

The RPT as [23] is used to derive the DKdVB equation in unmagnetised collisional dusty plasma to study the nonlinear wave propagation of DIAWs. The independent variables are stretched as [24]

(6){ξ=ε1/2(xvt)τ=ε3/2t

where ε is the strength of nonlinearity, and v is the phase velocity of the DIAWs to be determined from the lowest order of ε. The expansions of the dependent variables n,u,ϕ,η,νid are as follows:

(7){n=1+εn1+ε2n2+,u=0+εu1+ε2u2+,ϕ=0+εϕ1+ε2ϕ2+,η=ε1/2η0,νidε3/2νid0.

Substituting the above expansions (7) along with stretching coordinates (6) into (1) to (3) and equating the coefficients of the lowest order of ε, the dispersion relation is obtained as

(8)v=1a(1μ),

with a=q+12.

Taking the coefficients of the next higher order of ε, we obtain the DKdVB equation

(9)ϕ1τ+Aϕ1ϕ1ξ+B3ϕ1ξ3+C2ϕ1ξ2+Dϕ1=0,

where A=(32vv3(1μ)b), B=v32, C=η102, and D=νid02 with b=(q+1)(3q)8.

In absence of C and D, i.e. for C = 0 and D = 0, (9) takes the form of well-known KdV equation with the solitary wave solution

(10)ϕ1=ϕmsech2(ξM0τW),

where amplitude of the solitary waves ϕm=3M0A and width of the solitary waves W=2BM0, with M0 is the speed of the ion-acoustic solitary waves or Mach number.

It is well established for the KdV equation that

(11)I=ϕ12dξ

is a conserved quantity [25].

For small values of C and D, let us assume that amplitude, width, and velocity of the ion acoustic waves are dependent on τ [26], [27], [28], [29], and the slow time-dependent solution of (9) is of the form

(12)ϕ1=ϕm(τ)sech2(ξM(τ)τW(τ)),

where the amplitude ϕm(τ)=3M(τ)A, width W(τ)=2B/M(τ), and velocity M(τ) have to be determined.

Differentiating (11) with respect to τ and using (9), one can obtain

(13)dIdτ+2DI=2C(ϕ1ξ)2dξ,
(14)dIdτ+2DI=2C×245M5/2(τ)A2B.

where

(15)(ϕ1ξ)2dξ=245M5/2(τ)A2B

and

(16)I=ϕ12dξ,I=ϕm2(τ)sech4(ξM(τ)τW(τ))dξ,I=24BA2M3/2(τ).

Substituting (16) and (15) into (14), we obtain

(17)dM(τ)dτ+PM(τ)=QM2(τ),

which is the Bernoulli’s equation, where P=43D and Q=415CB.

The solution of (17) is

M(τ)=PM0M0Q(1ePτ)+PePτ

Therefore, the slow time dependence form of the ion-acoustic solitary wave solution of the DKdVB (9) is given by (12) where M(τ)=PM0M0Q(1ePτ)+PePτ and M(0)=M0 for τ = 0.

4 Effects of Parameters

The effects of the parameters, i.e. ion collision frequency parameter (νid0), the entropic index (q), time (τ), ratio of unperturbed number densities of electrons and ions (μ), viscosity coefficient (η10), and Mach number (M0) on the solitary wave solution of the DKdVB (9), have been studied in this section.

In Figure 1, the soliton solution of the DKdVB equation is plotted from (12) for different values of the dust ion collision frequency parameter (νid0). The values of other parameters are μ=0.5,q=0.6,τ=2,η10=0.1,M0=0.1. It is observed that the solution produces solitary waves, and the amplitude of the solitary waves decreases as the value of the parameter νid0 increases and the width of the solitary waves increases for increasing value of νid0. To show the variation of the amplitude and width of the solitary wave with respect to the dust ion collision frequency, Figures 2 and 3 are plotted.

Figure 1: Variation of solitary wave from (12) for the different values of νid0\({\nu_{id0}}\) with M0 = 0.1, q = 0.6, τ = 2, η10=0.1\({\eta_{10}}=0.1\), and μ = 0.5.
Figure 1:

Variation of solitary wave from (12) for the different values of νid0 with M0 = 0.1, q = 0.6, τ = 2, η10=0.1, and μ = 0.5.

Figure 2: Variation of the amplitude of the solitary wave from (12) with respect to νid0\({\nu_{id0}}\) and all other parameters are the same as Figure 1.
Figure 2:

Variation of the amplitude of the solitary wave from (12) with respect to νid0 and all other parameters are the same as Figure 1.

Figure 3: Variation of width of the solitary wave from (12) with respect to νid0\({\nu_{id0}}\) and all other parameters are the same as Figure 1.
Figure 3:

Variation of width of the solitary wave from (12) with respect to νid0 and all other parameters are the same as Figure 1.

In Figure 2, the amplitude of the solitary wave is plotted with respect to the collision frequency parameter (νid0), and it is obvious that the amplitude of the solitary wave decreases as the dust ion collision frequency parameter (νid0) increases gradually for positive nonzero values, and the other parameters remain the same as those in Figure 1, and for νid0=0, the solitary wave solution does not exist.

In Figure 3, the width of the solitary wave is plotted, and it is obvious that the width of the solitary wave increases as the dust ion collision frequency parameter (νid0) increases gradually for positive nonzero values and the other parameters remain the same as those values in Figure 1, and for νid0=0, the solitary wave does not exist. That is why the figure does not show any amplitude and width of the solitary wave in case of νid0=0. In absence of dust ion collision, (9) reduces to planar KdVB equation, and its solution does not produce solitary wave.

In Figure 4, the solution of the DKdVB equation is plotted from (12) for different values of the nonextensive parameter (q). The other parameters are μ=0.5,τ=2,η10=0.1,M0=0.1 and νid0=.01. The figure shows that the amplitude and width of the solitary waves decrease as the value of the nonextensive parameter q increases for fixed dust ion collision and other parameters.

Figure 4: Variation of solitary wave from (12) for the different values of q with M0 = 0.1, τ = 2, η10=0.1\({\eta_{10}}=0.1\), νid0=0.01\({\nu_{id0}}=0.01\), and μ = 0.5.
Figure 4:

Variation of solitary wave from (12) for the different values of q with M0 = 0.1, τ = 2, η10=0.1, νid0=0.01, and μ = 0.5.

In Figure 5, the solution is plotted from (12) for different values of the parameter μ, where μ=n0en0i, i.e. ratio of unperturbed number densities of electrons and ions, and the other parameters are q=0.6,τ=2,η10=0.1,M0=0.1,νid0=0.01. It is observed that both the amplitude and width of the solitary waves decrease as the value of the ratio of the parameter number of unperturbed electrons and ions increases for fixed dust ion collision.

Figure 5: Variation of solitary wave from (12) for the different values of μ with q = 0.6, M0 = 0.1, τ = 2, η10=0.1\({\eta_{10}}=0.1\), and νid0=0.01\({\nu_{id0}}=0.01\).
Figure 5:

Variation of solitary wave from (12) for the different values of μ with q = 0.6, M0 = 0.1, τ = 2, η10=0.1, and νid0=0.01.

In Figure 6, the solitary wave solution is depicted from (12) for different values of the viscosity coefficient parameter of plasma (η10). The other parameters are μ=0.5,q=0.6,τ=2,νid0=0.01,M0=0.1. The viscosity coefficient (η10) plays an important role on the dust ion-acoustic solitary waves (DIASWs). The variation of the amplitude and width of the solitary waves with respect to (η10) is obvious from the next two consecutive figures.

Figure 6: Variation of solitary wave from (12) for the different values of η10 with q = 0.6, τ = 2, M0 = 0.1, νid0=0.01\({\nu_{id0}}=0.01\), and μ = 0.5.
Figure 6:

Variation of solitary wave from (12) for the different values of η10 with q = 0.6, τ = 2, M0 = 0.1, νid0=0.01, and μ = 0.5.

Figure 7 represents the variation of the amplitude of the solitary wave solution of DKdVB equation with respect to the coefficient of viscosity η10. It is seen that the amplitude of the solitary waves decreases monotonically if the values of the viscosity coefficient η10 increase gradually.

Figure 7: Variation of the amplitude of the solitary wave from (12) with respect to η10 for q = 0.6, τ = 2, M=0.1\({M_{=}}0.1\), νid0=0.01\({\nu_{id0}}=0.01\), and μ = 0.5.
Figure 7:

Variation of the amplitude of the solitary wave from (12) with respect to η10 for q = 0.6, τ = 2, M=0.1, νid0=0.01, and μ = 0.5.

Figure 8 shows the variation of the width of the solitary wave solution of DKdVB equation with respect to the viscosity coefficient η10. It is obvious that the width of the solitary waves increases monotonically if the value of the viscosity coefficient η10 increases gradually.

Figure 8: Variation of width of the solitary wave from (12) with respect to η10 for q = 0.6, τ = 2, M0 = 0.1, νid0=0.01\({\nu_{id0}}=0.01\), and μ = 0.5.
Figure 8:

Variation of width of the solitary wave from (12) with respect to η10 for q = 0.6, τ = 2, M0 = 0.1, νid0=0.01, and μ = 0.5.

In Figure 9, the solitary wave solution from (12) is plotted for different values of the time parameter τ, and the other parameters are μ=0.5,q=0.6,η10=0.1,νid0=0.01,M0=0.1. It is seen that the amplitude and width of the solitary waves change as the time (τ) is changed. The variation of the amplitude and width of the solitary waves with respect to the time (τ) is shown in the next two figures.

Figure 9: Variation of solitary wave from (12) for the different values of τ with q = 0.6, η10=0.1\({\eta_{10}}=0.1\), M0 = 0.1, νid0=0.01\({\nu_{id0}}=0.01\), and μ = 0.5.
Figure 9:

Variation of solitary wave from (12) for the different values of τ with q = 0.6, η10=0.1, M0 = 0.1, νid0=0.01, and μ = 0.5.

In Figure 10, the variation of the amplitude of the solitary wave solution of DKdVB equation with respect to time (τ) has been depicted. It is seen that the amplitude of the solitary waves decreases as the time τ increases gradually when dust ion collision and other parameters are fixed.

Figure 10: Variation of the amplitude of solitary wave from (12) with respect to τ and the other parameters are μ=0.5,q=0.6,η10=0.1,νid0=0.01,M0=0.1\(\mu=0.5,q=0.6,{\eta_{10}}=0.1,{\nu_{id0}}=0.01,{M_{0}}=0.1\).
Figure 10:

Variation of the amplitude of solitary wave from (12) with respect to τ and the other parameters are μ=0.5,q=0.6,η10=0.1,νid0=0.01,M0=0.1.

In Figure 11, it is obvious that the width of the solitary waves increases as the time τ increases gradually.

Figure 11: Variation of the width of solitary wave from (12) with respect to τ and the other parameters are μ=0.5,q=0.6,η10=0.1,νid0=0.01,M0=0.1\(\mu=0.5,q=0.6,{\eta_{10}}=0.1,{\nu_{id0}}=0.01,{M_{0}}=0.1\).
Figure 11:

Variation of the width of solitary wave from (12) with respect to τ and the other parameters are μ=0.5,q=0.6,η10=0.1,νid0=0.01,M0=0.1.

It is clear from Figure 12 that the amplitude of the solitary wave increases and the width of the solitary wave decreases as the value of the Mach number increases. Thus, Mach number plays an important role on the variation of the amplitude and width of the solitary waves. Hence, we can conclude that the subsonic and supersonic waves exist in the framework of the DKdVB equation.

Figure 12: Variation of solitary wave from (12) for the different values of M0 with q = 0.6, η10=0.1\({\eta_{10}}=0.1\), τ = 2, νid0=0.01\({\nu_{id0}}=0.01\), and μ = 0.5.
Figure 12:

Variation of solitary wave from (12) for the different values of M0 with q = 0.6, η10=0.1, τ = 2, νid0=0.01, and μ = 0.5.

From the above description, it is seen that solitary wave solution exists for the small values of the parameters involved in the coefficients of the dissipation and damping terms in the DKdVB equation. Although for the planar KdVB equation solitary wave solution does not exist, the solution of the planar KdVB equation exhibits either the transition of a monotonic to oscillatory shock wave or the transition of an oscillatory to monotonic shock wave, depending on the parameters of the system. In this article, it is observed that the proper balancing of the dispersion term with dissipation and damping produces solitary waves.

5 Conclusions

In this article, we have studied the effects of the different parameters on the DIASWs in a dusty plasma with negatively charged ions, nonextensive electron, and stationary dust particles. The RPT is employed to derive the DKdVB equation. This is the first time analytical solution has been derived in the framework of DKdVB equation for the small values of the coefficient of dissipation and damping. The effects of the parameters dust ion collision (νid0), the entropic index q, Mach number (M), coefficient of viscosity (η10), the ratio between the unperturbed densities of the electrons and ions (μ), and time (τ) on the amplitude and width of the DIASWs solution have been investigated. It is seen that the parameters have played an important role on the shape of the DIASWs in a collisional dusty plasma. The results may be useful in laboratory plasmas as well as space environments where q-nonextensive distributed electrons are present.

Acknowledgements

The authors thank the reviewers for their valuable suggestions and comments, which help to improve the quality of the article. Also, the authors are grateful to Dr. Asit Saha, Sikkim Manipal Institute of Technology, Sikkim Manipal University, Majitar, Rangpo, East-Sikkim 737136, India, for his kind cooperation.

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Received: 2018-11-25
Accepted: 2019-04-23
Published Online: 2019-05-22
Published in Print: 2019-09-25

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