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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Bibliographic Details
Main Authors: Noreen, N, Shiekh, A, Habumugisha, I, Zaheer, S, AShah, H
Format: Article
Language:en_US
Published: IOP Publishing 2020
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Online Access:http://hdl.handle.net/20.500.12493/420
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