Central explosion in an equilibrium inhomogeneous sphere in its own gravitational field

Details Central explosion in an equilibrium inhomogeneous sphere in its own gravitational field Central explosion in an equilibrium inhomogeneous sphere in its own gravitational field

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr......179c&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Mekhanika Zhidkosti i Gaza (ISSN 0568-5281), May-June 1988, p. 179-184. In Russian.

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Computation

Computational Astrophysics, Gas Explosions, Gravitational Fields, Shock Waves, Stars, Supernovae, Asymptotic Methods, Equilibrium, Gas Dynamics, Gravitational Collapse, Inhomogeneity, Shock Layers

Scientific paper

The paper is concerned with the non-self-similar problem of the central explosion of an equilibrium inhomogeneous gas sphere in its own gravitational field. The problem, which is relevant to the study of stellar phenomena and particularly supernova explosions, is solved by the asymptotic method of a thin shock layer. It is shown that, with a sufficiently high explosion energy, after the shock wave has reached the surface of the sphere, the initially inhomogeneous self-gravitating gas sphere (star) will expand into the void (interstellar medium) completely, without any central gravitational residue left.

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