Non-rigid massive spheres in general relativity

Details Non-rigid massive spheres in general relativity Non-rigid massive spheres in general relativity

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192..659d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 192, Sept. 1980, p. 659-662. Research supported by the University Grant

Computer Science

Sound

11

Neutron Stars, Relativity, Stellar Mass, Stellar Models, Stellar Structure, Density Distribution, Equations Of State, Spheres

Scientific paper

Solutions corresponding to spheres with a slowly varying density (proportional to 1 - the ratio of the square of the radius to the square of the size of the sphere times the rigidity parameter) are evaluated. This has been applied to construct a model of a neutron star. The mass of a neutron star comes out to be 3.34 solar masses, when everywhere the speed of sound remains less than the speed of light. Under extreme conditions the mass of a neutron star approaches the limit of 8 solar masses. The mass/radius ratio for the physical condition P = 1/3 the density comes out to be more than that for a constant density sphere.

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