999精品在线视频,手机成人午夜在线视频,久久不卡国产精品无码,中日无码在线观看,成人av手机在线观看,日韩精品亚洲一区中文字幕,亚洲av无码人妻,四虎国产在线观看 ?

Electron acoustic solitary waves in unmagnetized nonthermal plasmas

2021-05-13 07:06:06MuhammadKhalidAqilKhanMohsinKhanDaudKhanSherazAhmadandAtaurRahman
Communications in Theoretical Physics 2021年5期

Muhammad Khalid,Aqil Khan,Mohsin Khan,Daud Khan,Sheraz Ahmad and Ata-ur-Rahman

1 Department of Physics,Government Post Graduate College Mardan,Mardan 23200,Pakistan

2 Theoretical Plasma Physics Group,Department of Physics,Islamia College Peshawar (Public Sector University),Peshawar 25120,Pakistan

3 Department of Physics,Government Post Graduate College Nowshera,Nowshera 24100,Pakistan

Abstract Electron acoustic (EA) solitary waves (SWs) are studied in an unmagnetized plasma consisting of hot electrons(following Cairns-Tsalli distribution),inertial cold electrons,and stationary ions.By employing a reductive perturbation technique (RPT),the nonlinear Korteweg-de Vries(KdV) equation is derived and its SW solution is analyzed.Here,the effects of plasma parameters such as the nonextensivity parameter(q),the nonthermality of electrons(α),and the cold-to-hot electron density ratio (β) are investigated.

Keywords: Electron acoustic solitons,KdV equation,Cairns-Tsalli distribution

1.Introduction

In plasmas,electron acoustic waves (EAWs) contains hot inertialess electrons and cold inertial electrons.When inertial cold electrons oscillate,EAWs are produced,in contrast to inertialess hot electrons.Watanbe and Taniuti showed that if electrons in plasma have two different temperatures,i.e high and low,then an electron acoustic mode occurs.When the number density of hot electrons is smaller than that of those at lower temperatures,the electron acoustic mode is damped(landau),while in the opposite case,solitary waves(SWs)can be propagated [1].Yu and Shukla studied low-temperature cold-electron density and concluded that it strongly depended on frequency [2].They also discussed the solitons that are associated with modified EAWs.The topological behaviour of higher order modes (HOMs) in two-electron-temperature plasmas and the conditions under which HOMs can become weakly damped were qualitatively studied by Mace and Hellberg [3].The existence of modulational instabilities and also the occurrence of envelope solitary structures involving EAWs that propagate in unmagnetized plasma,which consist of cold electrons,hot electrons,and ions,meant that three components of plasma were discussed in [4].There are numerous differential equations that are used to describe many linear and nonlinear natural phenomena in different media such as shallow water,nonlinear optics,and plasma [5-12].

The study of nonlinear periodic waves has gained considerable interest within plasma physics; some examples are mentioned in[4,13-21].The properties of EAWs that propagate obliquely in magnetized plasmas composed of a cold magnetized electron fluid and a hot vortex-like distribution of electrons and ions were discussed by Mamun and Shukla,they studied the effects of the external magnetic field and obliqueness and found that they changed important properties of EAWs,such as amplitude and width [21].The electrostatic modes in an unmagnetized and homogenous plasma of three Maxwellian components: ions,hot electrons and cold electronswere studied by Gary and Tokar[22].Baluku et al[23]investigated EAWs in a plasma whose electron-velocity distribution was a combination of two kappa κ distributions with different densities,temperatures and values of kappa κ,using kinetic theoretical approach.They concluded that when the hot and cold densities became equal,then the damping of EAWs in this region was very small.Lu et al performed a 1D particle in cell electrostatic stimulation to analyze the nonlinear evolution of electrostatic waves excited in an unmagnetized plasma which was composed of cold,hot and beam electrons [24].Shukla et al [25] performed a theoretical investigation which helped to confirm the properties of multidimensional(3D)electron acoustic solitary waves(EASWs)in a magnetized plasma composed of stationary ions and magnetized cold electrons with an amount of beam electrons and magnetized hot electrons which obeyed a vortex-like distribution.They derived and mathematically solved a modified 3D KdV equation and concluded that 3D EASWs evolve with time.Younsi and Tribeche [26] showed the occurrence of arbitrary amplitude EA solitary potentials in a plasma composed of ions,cold electrons (inertial) and hot superthermal electrons.They concluded that localized EASWs can exist in such plasmas.They also found out that when the superthermal character of plasma increases,the potential pulse amplitude also increases,but its width becomes narrower.Moreover,the superthermal effect makes the EA solitary structures more spiky.In this paper,we describe a search for the propagation of EAWs in a plasma consisting of Cairns-Tsalli distributed hot electrons,inertial cold electrons and stationary ions.

This paper is organized as follows: model equations are given in section 2; the linear dispersion relation is derived in section 3;the derivation of the KdV equation by RPT and its SW solution are presented,respectively,in sections 4 and 5;a discussion is offered in section 6.In section 7,the conclusions of our work are presented.

2.Basic equations

We consider a three-component plasma comprising cold electrons,hot electrons and stationary ions.The hot electrons follow a nonthermal distribution,inertial cold electrons and the ions are stationary in the background.The dynamics of the cold electrons are governed by the following set of normalized equations:

The hot electrons are assumed to follow Cairns-Tsalli distribution [27,28],given by:

where we define

and

where q is a real parameter,known as nonextensivity [29],and α is a real parameter associated with the number of nonthermal electrons in the distribution [30].Here,nc(nh) is the cold (hot) electron number density scaled by its equilibrium value nc0(nh0),ucis the cold electron fluid velocity scaled by the EA speedandis the normalized electrostatic wave potential.The space variable (x)and time variable (t) are scaled byandrespectively.The cold-to-hot electron density ratio,The subscript ‘c’ is dropped from the rest of calculation for simplicity.

For φ ? 1,equation(4)can be expanded in the power of the potential as,

where c1and c2are defined,respectively,asc1=andUsing equation (7) in equation (3),we obtain

3.Linear analysis

Following the method provided in [27],we linearize equations (1)-(3) using a standard procedure where the firstorder quantities are proportional to exp (ikx- iωt),thus we obtain a linear dispersion relation in the form of

where c1is defined above.

4.Derivation of the KdV equation

To derive the KdV equation,we should adopt the RPT.The stretching of coordinates is given as

where vphis the EA speed and is interpreted as the phase velocity,and ∈is a very small real parameter.

Expanding the dependant variables as follows,

Using (10) and (11) in equations (1),(2),and (8) gives the first order quantities as

and

Comparing equations (12) and (14),we get

Moving to the next order of ∈i.e.the second order perturbation,we get

Now solving equations (16)-(18) and making the use of first order quantities,we get

where φ1≡ φ.This is the KdV equation for EA waves,where the nonlinear coefficient A and the dispersion coefficient B are given below:

5.The SW solution

To solve equation (19),we define a traveling-wave transformation η = ? - v0τ,in respect of which the wave is stationary,where v0is the velocity of the EASW.Using this transformation,equation (19) takes the following form

By solving the above equation using integration and some mathematical steps,we get

6.Numerical analysis

To study the behaviour of EASWs,we have derived the KdV equation,which we use to study the effects of various parameters involved in the coefficients of the KdV equation.These effects are studied with the help of various graphs that are discussed below.

Figure 1.Plots of ω(k) versus k,for different values of: (a)nonextensivity parameter q;(b)nonthermality parameter α;(c)coldto-hot electron density ratio parameter β.

If we take into account the dispersion relation equation (9),the value of ω is strongly dependent upon the value of k.As shown in figure 1,ω increases as the value of k increases.A discussion of the ω-k graph depends upon c1,which is a further function of α,q and β.Figure 1(a) shows that whenever the value of q increases,a decrease occurs in the ω-k graph.This means that ω is inversely proportional to the parameter q.On the other hand,figure 1(b) shows the effect of α parameter on the ω-k graph.When the value of α increases,the graph also increases,as shown in the figure.Therefore,it shows a direct relation.Figure 1(c) shows the effect of β.As it is clear from equation (9),ω increases with an increase in the value of β,that is why the effect of β on the ω-k graph shows a direct variation,i.e.whenever β increases,the graph also changes to a higher value on the ω axis,as shown in figure.

Figure 2.Variation of vph versus β for different values of: (a) the nonextensivity parameter q; (b) the nonthermality parameter α.

We now discuss the phase velocity of EASWs as given by equation(15).From the equation,it is clear that the phase velocity is directly proportional to β and inversely proportional to c1,which leads our discussion to study the effects of the parameters α,q and β on vph.Figure 2 presents the vph-β graph,which shows that the phase velocity increases as the value of β increases.Figure 2(a) shows that the q parameter has an inverse response to the vph- β graph,similarly α also affects the phase velocity: if α increases then the graph decreases.The effects of α and q parameters on the vph-β graph are shown in figures 2(a) and (b).

Moving to a study of the EASW,the nonlinear coefficient,A,and the dispersion coefficient,B,present in the KdV equation (19) are functions of various relevant plasma parameters.These parameters affect the structural characteristics of the pulses and may therefore lead to the generation of various kinds of EA solitary structures in a given plasma system.Figure 3 shows the SW solution for φ(η) versus η.Only negative pulses have been observed for the given plasma parameters α, q,and β.Figure 3(a)shows the effect of the q parameter on EASWs; if the value of q increases,both amplitude and width of the soliton decreases.The dependency of the SWs on α parameter is shown in figure 3(b).If we increase the value of α then the amplitude of the soliton decreases while its width increases,as shown in the figure.A similar situation occurs in case of β.An increase in β has the result that the amplitude of the soliton decreases,while its width increases,as shown in figure 3(c).

Figure 3.Variation ofφ (η) versus η for different values of: (a) the nonextensivity parameter q; (b) the nonthermality parameter α; (c)the cold-to-hot electron density ratio parameter β,with v0 = 0.1.

7.Conclusions

The propagation of EASWs was studied in an unmagnetized plasma consisting of hot electrons (following Cairns-Tsalli distribution),inertial cold electrons,and stationary ions.By employing RPT,the nonlinear KdV equation was derived and its SW solution was analyzed.The effects of plasma parameters such as the nonextensivity parameter (q),the nonthermality of electrons (α),and the cold-to-hot electron density ratio (β) were investigated.

Due to the variation of α, q and β,the KdV equation only gave the negative potential EA solitary structures for a given plasma system.It was found that smaller(in amplitude)and wider (in width) wave structures were obtained with increasing values of α and β.Also,smaller and narrower solitary structures were obtained with increasing values of q.

This work may be helpful in various space observation and astrophysical environments,where nonthermal nonextensive electrons are present [31,32].

主站蜘蛛池模板: 免费在线成人网| 亚洲黄网在线| 中文字幕亚洲乱码熟女1区2区| 99激情网| 欧美一级色视频| 日韩第一页在线| 国产免费自拍视频| 在线国产你懂的| 久久夜夜视频| 欧美精品在线看| 蜜臀AVWWW国产天堂| 波多野衣结在线精品二区| 欧美www在线观看| 免费高清a毛片| 午夜精品区| 97国产成人无码精品久久久| 日韩在线永久免费播放| 国产成人亚洲精品色欲AV | 亚洲综合经典在线一区二区| 玖玖精品在线| 成人福利在线视频| 亚洲浓毛av| 好紧好深好大乳无码中文字幕| 亚洲狠狠婷婷综合久久久久| 又黄又湿又爽的视频| 人妻精品全国免费视频| 精品少妇人妻av无码久久| 免费国产不卡午夜福在线观看| 国产制服丝袜无码视频| 鲁鲁鲁爽爽爽在线视频观看| 真人高潮娇喘嗯啊在线观看| 五月天婷婷网亚洲综合在线| 国内a级毛片| 亚洲人成影院在线观看| 五月婷婷精品| 亚洲日本精品一区二区| 少妇高潮惨叫久久久久久| 亚洲欧美日韩中文字幕在线一区| 一级香蕉视频在线观看| 日韩国产精品无码一区二区三区| 深夜福利视频一区二区| 亚洲高清无码久久久| aa级毛片毛片免费观看久| 伊人查蕉在线观看国产精品| 国产精品无码一二三视频| 国产午夜无码专区喷水| 日韩最新中文字幕| 亚洲精品国产日韩无码AV永久免费网 | 99久久精品国产麻豆婷婷| 伊人久久大线影院首页| 国产激情无码一区二区APP | 日本一本正道综合久久dvd| 亚洲国产精品成人久久综合影院| 精品無碼一區在線觀看 | 香蕉eeww99国产在线观看| 久久鸭综合久久国产| 伊人久热这里只有精品视频99| 91探花国产综合在线精品| 亚洲人成网站色7799在线播放| 日韩欧美中文亚洲高清在线| 国产亚洲视频播放9000| 亚洲国产成人在线| 91青青草视频| 亚洲香蕉在线| 久久网欧美| 91国内在线观看| 成人噜噜噜视频在线观看| 亚洲国产精品久久久久秋霞影院| 久久久国产精品无码专区| 秋霞国产在线| 亚洲欧美一区二区三区图片 | 一级毛片网| 99无码中文字幕视频| 日韩AV无码一区| 亚洲欧洲日韩综合| 亚洲一级毛片在线观播放| 久久77777| 亚洲天堂啪啪| 夜精品a一区二区三区| a级毛片免费网站| 欧美区一区| 青青青国产精品国产精品美女|