Model neutron stars with a constant scalar field in the bimetric scalar-tensor theory of gravitation. Different versions of the equation of state.

Details Model neutron stars with a constant scalar field in the bimetric scalar-tensor theory of gravitation. Different versions of the equation of state. Model neutron stars with a constant scalar field in the bimetric scalar-tensor theory of gravitation. Different versions of the equation of state.

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap.....41..194g&link_type=abstract

Astrophysics, Volume 41, Issue 2, pp.194-197

Astronomy and Astrophysics

Astrophysics

Neutron Stars: Equation Of State, Neutron Stars: Scalar-Tensor Theory

Scientific paper

In our preceding paper we found solutions for the equations of the bimetric scalar—tensor theory of gravitation for neutron stars, in which the scalar field is constant while the metric tensor satisfies the equations of the general theory of relativity. In the present paper we find analogous solutions for different versions of the equation of state of the matter of a neutron star.

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