Gravitational collapse of a radiating shell of matter

Details Gravitational collapse of a radiating shell of matter Gravitational collapse of a radiating shell of matter

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvd..31..233p&link_type=abstract

Physical Review D (Particles and Fields), Volume 31, Issue 2, 15 January 1985, pp.233-240

Physics

8

Fundamental Problems And General Formalism, Late Stages Of Stellar Evolution

Scientific paper

The nonstationary collapse of a radiating fluid shell of matter has been followed through its event horizon in the Vaidya metric in terms of Israel coordinates. The surface density and pressure of the shell were obtained from the integration of the collapse history and are displayed as functions of the shell radius. The shell behavior is determined by two free parameters: its mass function and luminosity-radius relationship. The effects of varying the forms of these two functions have also been examined.

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