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- W2081183663 abstract "Gamma-ray bursts are thought to come from a relativistic blast-wave emitting gamma-rays at a distance of 10 to 1000 AU from the central engine which releases the explosive energy. To account for the observed duration and variability of GRBs, the central engine powering the γ-ray emission must be active from several to many seconds and yet must strongly fluctuate in its output on much shorter timescales. A differentially rotating neutron star of millisecond period and canonical magnetization (DROMP) will wind up a toroidal magnetic field of >1016 G and then will release its magnetic energy, E∼1051 erg, in a rapid sub-burst. This process will repeat on a timescale of t∼1 to 103 s (depending on the initial conditions) until the kinetic energy of differential rotation is exhausted after several (N) sub-bursts. The calculated values E, t, N are in agreement with observations. The baryon loading in each sub-burst was found to be also in agreement with theoretical requirements for cosmological GRBs. DROMPs would..." @default.
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- W2081183663 date "1998-01-01" @default.
- W2081183663 modified "2023-09-25" @default.
- W2081183663 title "The physical source of gamma-ray bursts" @default.
- W2081183663 doi "https://doi.org/10.1063/1.55456" @default.
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