Neutron star in presence of torsion-dilaton field

Details Neutron star in presence of torsion-dilaton field Neutron star in presence of torsion-dilaton field

1998-03-26

arxiv.org/abs/gr-qc/9803084v3

Class.Quant.Grav.16:2359-2380,1999

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

29 pages, latex, 24 figures, final version. Added: 1)comments on different possible mass definitions; 2)new sections: a)the in

Scientific paper

10.1088/0264-9381/16/7/314

We develop the general theory of stars in Saa's model of gravity with propagating torsion and study the basic stationary state of neutron star. Our numerical results show that the torsion force decreases the role of the gravity in the star configuration leading to significant changes in the neutron star masses depending on the equation of state of star matter. The inconsistency of the Saa's model with Roll-Krotkov-Dicke and Braginsky-Panov experiments is discussed.

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