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- W2029389699 startingPage "2232" @default.
- W2029389699 abstract "In this Letter we investigate the possibility of Langmuir turbulence generation by directed gamma rays penetrating a background plasma. Turbulence is generated because Compton scattering creates superthermal electrons whose distribution can be unstable to the Cherenkov radiation of Langmuir waves. Using the Klein-Nishina cross section for relativistic Compton scattering, we calculate the momentum distribution of recoil electrons and derive the increment of instability for nonmagnetized plasma. The instability appears when there is a sufficiently narrow bump, for example, annihilation line $hensuremath{nu}{phantom{rule{0ex}{0ex}}=phantom{rule{0ex}{0ex}}m}_{e}{c}^{2}$ with a width less than $0.3{m}_{e}{c}^{2}$, in the gamma spectrum." @default.
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- W2029389699 date "1995-03-20" @default.
- W2029389699 modified "2023-09-26" @default.
- W2029389699 title "Instability of Langmuir Waves in Plasma Irradiated by Directed Gamma Rays" @default.
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- W2029389699 doi "https://doi.org/10.1103/physrevlett.74.2232" @default.
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