Exact relativistic model for a superdense star

Details Exact relativistic model for a superdense star Exact relativistic model for a superdense star

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982japa....3..325v&link_type=abstract

Journal of Astrophysics and Astronomy, vol. 3, Sept. 1982, p. 325-334.

Astronomy and Astrophysics

Astrophysics

45

Einstein Equations, Neutron Stars, Relativistic Theory, Stellar Models, Supermassive Stars, Astrophysics, Gravitational Collapse, Metric Space, Space-Time Functions, Stellar Evolution, Stellar Gravitation

Scientific paper

The gravitational significance of space-times which have hypersurfaces t = const as 3-spheroids is investigated. These space-times are utilized to develop static models which describe the gravitational field in the interior of superdense condensations of matter like white dwarfs and neutron stars. A static spherically symmetric model based on an exact solution of Einstein's equations is developed which permits densities of the order of 2 x 10 to the 14th g/cu cm, radii of the order of a few kilometers, and masses up to about four times the solar mass.

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