Physics
Scientific paper
Feb 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998prama..50...95t&link_type=abstract
Pramāna, Vol. 50, No. 2, p. 95 - 103
Physics
12
Relativistic Stars: Superdense Matter, Relativistic Stars: Stability
Scientific paper
A new exact closed form solution of Einstein's field equations is reported describing the space-time in the interior of a fluid sphere in equilibrium. The physical 3-space, t = constant of its space-time has the geometry of a 3-pseudo spheroid. The suitability of this solution for describing the model of a relativistic superdense star is discussed and the stability of the model under radial pulsations is examined.
Thomas V. O.
Tikekar Ramesh
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