Abstract
Velocity distribution functions with an excess of superthermal particles are commonly observed in space plasmas, and are effectively modeled by a kappa distribution. They are also found in some laboratory experiments. In this paper we obtain existence conditions for and some characteristics of ion-acoustic solitary waves in a plasma composed of cold ions and κ -distributed electrons, where κ>3/2 represents the spectral index. As is the case for the usual Maxwell-Boltzmann electrons, only positive potential solitons are found, and, as expected, in the limit of large κ one recovers the usual range of possible soliton Mach numbers, viz., 1<M<1.58. For lower values of κ, modeling the presence of a greater superthermal component, the range of accessible Mach numbers is reduced. It is found that the amplitude of the largest possible solitons that may be generated in a given plasma (corresponding to the highest allowed Mach number for the given plasma composition) falls off with decreasing κ, i.e., an increasing superthermal component. On the other hand, at fixed Mach number, both soliton amplitude and profile steepness increase as κ is decreased. These changes are seen to be important particularly for κ<4, i.e., when the electrons have a "hard" spectrum.
Original language | English |
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Article number | 062903 |
Journal | Physics of Plasmas |
Volume | 16 |
Issue number | 6 |
DOIs | |
State | Published - 2009 |
Externally published | Yes |
Funding
Useful discussions with Thomas Baluku, Richard Mace, and Frank Verheest are gratefully acknowledged. The work of N.S.S. and I.K. was supported by a UK EPSRC Science and Innovation award in Plasma Physics (CPP grant EP/D06337X/1). N.S.S. would like to thank Guru Nanak Dev University, Amritsar, India for providing leave. Part of the work was carried out by I.K. during a research visit to the University of Sydney. I.K. is grateful to the UK Royal Society for the award of a travel grant, and to the University of Sydney for its hospitality and local support provided during that visit. The research is also supported in part by the National Research Foundation of South Africa (NRF). Any opinion, findings, and conclusions or recommendations expressed in this material are those of the authors and therefore the NRF does not accept any liability in regard thereto.
Funders | Funder number |
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EPSRC Science and Innovation | |
Engineering and Physical Sciences Research Council | EP/D06337X/1 |
Royal Society | |
National Research Foundation |