Neutron star in presence of torsion-dilaton field
نویسندگان
چکیده
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 and increases the maximum of the neutron star mass up to 5− 6M⊙ depending on the equation of state of matter. gr-qc/9803084
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