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- W68073423 abstract "In this article, magnetic reconnection caused by the instability of neutron star magnetosphere has been proposed as the electron acceleration mechanism in Gamma-ray bursts(GRBs). The beamed relativistic electrons accelerated directly by the acceleration mechanism inpulsively eject from the magnetic reconnection region approximately in the line of the magnetic field direction These electrons emit photons through synchrotron radiation and lose energy. The synchrotron radiation spectrum has been calculated, including the radiation loss. This kind of spectrum form is different from the known form of synchro tron radiation and satisfactorily fits the three successive continuum spectra and the time evolution of N_(14) (150—700KeV)/N_(13) (40—180KeV) in GB820828 showing remarkable spectral variability. Also the radiation mechanism can reasonably explain the common characteristics, i.e., the absorption and emission features only appear at the beginning of GRBs with fast spectral variability." @default.
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- W68073423 date "1992-09-01" @default.
- W68073423 modified "2023-09-23" @default.
- W68073423 title "Synchrotron radiation of the beamed particles and the spectral variability of gamma-ray bursts." @default.
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