期刊
INTERNATIONAL JOURNAL OF MODERN PHYSICS D
卷 19, 期 12, 页码 1889-1904出版社
WORLD SCIENTIFIC PUBL CO PTE LTD
DOI: 10.1142/S0218271810018098
关键词
Neutron stars; general relativity
资金
- U.G.C.
The relativistic equations governing the non-adiabatic shear-free collapse of massive superdense stars in the presence of dissipative forces producing heat flow in the background of space-times of the Vaidya-Tikekar ansatz with associated physical three-spaces that have the three-spheroidal geometry are formulated. It is shown how the system can be used to examine the development and progress of the collapse during subsequent epochs until the radiating star becomes a black hole.
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