Neutron stars in the bimetric scalar—tensor theory of gravitation. II. solutions with a variable scalar field

Details Neutron stars in the bimetric scalar—tensor theory of gravitation. II. solutions with a variable scalar field Neutron stars in the bimetric scalar—tensor theory of gravitation. II. solutions with a variable scalar field

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap.....41...85g&link_type=abstract

Astrophysics, Volume 41, Issue 1, pp.85-88

Astronomy and Astrophysics

Astrophysics

Scientific paper

Solutions of the equations of the bimetric scalar—tensor theory of gravitation with a variable scalar field are found for configurations of superdense matter with different versions of the equation of state. The possible existence of static superdense and supermassive configurations is established for all of the versions of the equation of state of superdense matter used.

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