A study is made of equilibrium neutron configurations with allowance for nuclear interactions and two theories of gravitation-Einstein's and the scalar-tensor. The equation of state of neutron matter is obtained on the basis of the model of single-boson exchange in the Hartree-Fock approximation. Various parameters of neutron stars are obtained and the influence of the choice of the coupling constant GρNN 2 and the masses of scalar mesons on these parameters investigated.
ASJC Scopus subject areas
- Physics and Astronomy(all)