Journal
INTERNATIONAL JOURNAL OF MODERN PHYSICS D
Volume 16, Issue 9, Pages 1479-1495Publisher
WORLD SCIENTIFIC PUBL CO PTE LTD
DOI: 10.1142/S0218271807010845
Keywords
gravitational collapse; superdense star; core-envelope models
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The non-adiabatic gravitational collapse of a spherical distribution of matter accompanied by radial heat flux has been studied on the background of a pseudo-spheroidal space-time. The spherical distribution is divided into two regions: a core consisting of anisotropic pressure distribution and an envelope consisting of isotropic pressure distribution. Various aspects of the collapse have been studied using both analytic and numerical methods.
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