Abstract
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 G 2ρNN and the masses of scalar mesons on these parameters investigated.
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 11, pp. 22–26, November, 1976.
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Reizlin, V.I. Equilibrium configurations of systems of neutrons with allowance for nuclear and gravitational interactions. Soviet Physics Journal 19, 1403–1406 (1976). https://doi.org/10.1007/BF00890782
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DOI: https://doi.org/10.1007/BF00890782