Gravitational field of a neutron star

Details Gravitational field of a neutron star Gravitational field of a neutron star

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982fiz....25...53e&link_type=abstract

Fizika, vol. 25, Jan. 1982, p. 53-57. In Russian.

Physics

Gravitational Fields, Neutron Stars, Stellar Gravitation, Energy Dissipation, Gravitation Theory, Ideal Fluids, Polarization (Spin Alignment)

Scientific paper

U4 gravitational theory is used to obtain internal and external solutions for the gravitational field of a neutron star consisting of an ideal fluid with axial spin-polarization. It is found that spin-spin interaction as described by U4 theory does not cause the appearance of a quadrupole moment which could be the source of appreciable gravitational radiation and thus of energy loss, manifested in the slow-down of stellar rotation.

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