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Properties of Relativistic Linear Stellar Models

Published online by Cambridge University Press:  12 April 2016

V. Ureche
V. Ureche*
Affiliation:
University of Cluj-Napoca, Cluj-Napoca, Romania

Extract

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In the late stages of stellar evolution, relativistic objects are formed, such as neutron stars or black holes. These relativistic stars possess a strong gravitational field, therefore their structure and their space-time geometry can be described only in the frame of GRT (Zeldovich and Novikov, 1971; Misner, Thorne and Wheeler, 1973). For this purpose, the following four-dimensional interval is used (spherical gravitational field), (Zeldovich and Novikov, 1971).

Type
Part I: Evolution of Stars in the Post-Main Sequence Stage
Information
International Astronomical Union Colloquium , Volume 69: Binary and Multiple Stars as Tracers of Stellar Evolution , 1982 , pp. 73 - 78
Copyright
Copyright © Reidel 1982

References

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