A Self-Similar Solution for Spherically Symmetric Gravitational Collapse

Details A Self-Similar Solution for Spherically Symmetric Gravitational Collapse A Self-Similar Solution for Spherically Symmetric Gravitational Collapse

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000astl...26..344a&link_type=abstract

Astronomy Letters, vol. 26, p. 344-355 (2000)

Astronomy and Astrophysics

Astronomy

3

Scientific paper

A model of gas-dynamical flow during gravitational collapse is analyzed mathematically by assuming its spherical symmetry and self-similarity. A shock wave diverging from the center emerges in this model. The physical requirements imposed on the post-shock flow at the center for the specified parameters at infinity unambiguously determine the shock front and the flow behind it.

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