Abstract
The papers deals with a model of origin of cosmic gamma-bursts (CGB) which appear at cosmological distances from the merging of two compact stars. The process of CGB degeneration is divided into three stages – formation of the initial state, hydrodynamic expansion and free runaway. Theory includes fundamental parameters – a star mass and electron mass. Quantitative predictions of a model agree with the observed characteristics of CGB.
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Rosental, I., Belousova, I. Origin of Cosmic Gamma-Bursts. Astrophysics and Space Science 249, 117–124 (1997). https://doi.org/10.1023/A:1000378029506
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DOI: https://doi.org/10.1023/A:1000378029506