Abstract
The internal and external solutions describing the gravitational field of a neutron star consisting of an ideal fluid with axially polarized spin are found within the framework of the metric-affine theory of gravitation under the approximation of weak gravitational and torsion fields.
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 1, pp. 53–57, January, 1982.
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Efremov, A.P. Gravitational field of a neutron star. Soviet Physics Journal 25, 51–55 (1982). https://doi.org/10.1007/BF00893875
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DOI: https://doi.org/10.1007/BF00893875