Rotating Neutron Stars in the Bi-Metric Theory of Gravitation

Details Rotating Neutron Stars in the Bi-Metric Theory of Gravitation Rotating Neutron Stars in the Bi-Metric Theory of Gravitation

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192...75f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 192, July 1980, p. 75-81. Research supported by the Fundacao de Amparo

Astronomy and Astrophysics

Astronomy

1

Equations Of State, Gravitation Theory, Neutron Stars, Stellar Models, Stellar Rotation, Logarithms, Moments Of Inertia, Red Shift, Relativistic Theory, Stellar Mass

Scientific paper

Rotating neutron stars properties are calculated according to the Bi-Metric Theory of Gravitation for a wide range of equations of state and compared with published results of the General Relativity Theory. It was found that the Bi-Metric Theory allows for appreciably higher masses, moments of inertia, and redshifts than the General Relativity Theory and that stable neutron stars can have: (1) masses greater than that of Cyg X-1, (2) moments of inertia of 10 to the 47th g sq cm or greater, and (3) maximum surface redshifts exceeding 4.

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