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Karpman-Washimi magnetization in relativistic quantum plasmas

Authors
Jamil, M.Rasheed, A.Usman, M.Arshad, W.Saif, M. JawwadJung, Young-Dae
Issue Date
Sep-2019
Publisher
AMER INST PHYSICS
Citation
PHYSICS OF PLASMAS, v.26, no.9, pp 1 - 7
Pages
7
Indexed
SCI
SCIE
SCOPUS
Journal Title
PHYSICS OF PLASMAS
Volume
26
Number
9
Start Page
1
End Page
7
URI
https://scholarworks.bwise.kr/erica/handle/2021.sw.erica/2160
DOI
10.1063/1.5096980
ISSN
1070-6631
1089-7666
Abstract
An interesting phenomenon of ponderomotive Karpman-Washimi magnetization is investigated in ultrarelativistic degenerate plasmas. The quantum characteristics of plasma electrons are considered on incorporating the Fermi pressure and exchange-correlation potential terms into the fluid model of plasmas. The ion fluid is referred to as classically warm. The Karpman-Washimi ponderomotive magnetization M-K-W(Str) and radiation power P-K-W(Str) are derived as functions of scaled wave number (k) over bar, scaled effective frequency (omega) over bar (*), ratio of thermal temperature of ions to the Fermi temperature of electrons (E) over bar (1)(P) , and fine structure constant alpha for two cases of streaming and nonstreaming quantum plasmas. It has been observed that the Karpman-Washimi ponderomotive magnetization M-K-W(Str) and the Karpman-Washimi radiation power P-K-W(Str) are significantly affected by the scaled streaming velocity (upsilon) over bar (0)
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ERICA 첨단융합대학 (ERICA 지능정보양자공학전공)
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