Linear analysis of bump on tail instability with non-Maxwellian distribution function
The growth rate of bump on tail instability propagating in unmagnetized plasma has been derived. The dispersion relation has been characterized for (r, q) distribution function with spectral indices r and q which ultimately contributes towards tails and shoulder of distribution function. The growt...
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Main Authors: | , , , , |
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Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2020
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Subjects: | |
Online Access: | http://hdl.handle.net/20.500.12493/420 |
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