Analytic neutron stars in general relativity - Exact solutions for the non-homogeneous charged model

Details Analytic neutron stars in general relativity - Exact solutions for the non-homogeneous charged model Analytic neutron stars in general relativity - Exact solutions for the non-homogeneous charged model

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..94..133i&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 94, no. 1, July 1983, p. 133-143.

Physics

3

Neutron Stars, Pulsars, Stellar Gravitation, Stellar Models, Equations Of State, Field Theory (Physics), Gravitation Theory, Stellar Rotation

Scientific paper

The Adams (1975) method for deriving analytical solutions to field equations for a spherically symmetric neutron star is extended to nonhomogeneous and rotating neutron stars (pulsars). It is shown that exchange processes on a rotating star can give rise to an electric field, and field equations are defined. Value ranges are defined for pulsar parameters that are consistent with observational evidence and theoretical predictions. A 0.01 contribution is demonstrated to be possible for the contribution of the electrical energy density to the total gravitational mass.

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