Friedmann-like collapsing radiating sphere

Details Friedmann-like collapsing radiating sphere Friedmann-like collapsing radiating sphere

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...342..976c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 342, July 15, 1989, p. 976-981.

Astronomy and Astrophysics

Astrophysics

7

Gravitational Collapse, Heat Transmission, Stellar Luminosity, Adiabatic Conditions, Geodesic Lines, Pressure Gradients, Schwarzschild Metric, Spheres

Scientific paper

The model of a collapsing body proposed by Kolassis et al. (1988) is further studied. Consideration is given to the collapse of a spherical body with a mass of 1.3 solar masses. Equations are solved in the weak flow approximation. There is a nonzero fluid pressure and, during the collapse, the pressure gradient becomes positive; this further increases the instability of the object.

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