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arXiv · 2208.11514

Explosion of a Minimum-Mass Neutron Star within Relativistic Hydrodynamics

A. V. Yudin
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Abstract

The relativistic hydrodynamics equations are adapted for the spherically symmetric case and the Lagrangian form. They are used to model the explosive disruption of a minimum-mass neutron star: a key ingredient of the stripping model for short gamma-ray bursts. The shock breakout from the neutron star surface accompanied by the acceleration of matter to ultrarelativistic velocities is studied. A comparison with the results of previously published nonrelativistic calculations is made.

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A. V. Yudin. 2022-08-23. Explosion of a Minimum-Mass Neutron Star within Relativistic Hydrodynamics. https://doi.org/10.1134/s106377372206007x

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