Neutron-star models in Ni's theory of gravity

Details Neutron-star models in Ni's theory of gravity Neutron-star models in Ni's theory of gravity

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.135..409s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 135, no. 2, July 1987, p. 409-415.

Astronomy and Astrophysics

Astrophysics

2

Gravitation Theory, Neutron Stars, Stellar Models, Stellar Structure, Approximation, Polytropic Processes, Stellar Gravitation, Stellar Mass

Scientific paper

For strongly gravitating systems such as massive neutron stars, structure equations of hydrostatic equilibrium have been derived in Ni's theory of gravity under a post-Newtonian approximation. Approximate analytical solution curves are given for neutron star models of polytropic indices n = 0 (a = 1, b = 1), n = 1 (a = 1, b = 1), and n = 2 (a = 2, b = 2; a = 1, b = 1). The physical significance of the maximum mass is briefly discussed.

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