Relativistic polytropic spheres in general relativity

Details Relativistic polytropic spheres in general relativity Relativistic polytropic spheres in general relativity

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.180...75p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 180, no. 1, June 1991, p. 75-92. Research supported by Council of Scientif

Statistics

Computation

Computational Astrophysics, Neutron Stars, Polytropic Processes, Relativistic Effects, Relativity, Spheres, Gravitational Effects, Metric Space, Red Shift, Stellar Models, Stellar Oscillations

Scientific paper

Spherical-symmetric massive structures with a relativistic polytropic equation of state have been studied in detail. The various static parameters have been calculated under all possible variations of sigma0 (which equals P0/E0, pertaining to the central value) and the polytropic index n. In particular, the values of the static parameters have been identified under the extreme relativistic conditions and for the most bound structures. The structures have been used to model neutron stars and the various neutron parameters have been calculated. Radial pulsation and rotation of these configurations have also been discussed.

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