Karpman-Washimi magnetization in relativistic quantum plasmas
- Authors
- Jamil, M.; Rasheed, A.; Usman, M.; Arshad, W.; Saif, M. Jawwad; Jung, 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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