Neutron gas of a degenerate superdense star with a frozen-in magnetic field

Details Neutron gas of a degenerate superdense star with a frozen-in magnetic field Neutron gas of a degenerate superdense star with a frozen-in magnetic field

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..101s&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, Jan.-Feb. 1991, p. 101-108. In Russian.

Astronomy and Astrophysics

Astronomy

10

Degenerate Matter, Neutron Stars, Stellar Magnetic Fields, Kinetic Energy, Magnetic Flux, Magnetic Moments

Scientific paper

The filling of the energy subbands of a degenerate nonrelativistic neutron gas of a superdense star is calculated as a function of the strength of the frozen-in magnetic field. It is shown that, as the magnetic field strength increases, the Fermi kinetic energy of the degenerate neutron gas increases to a limiting value, which corresponds to the filling by neutrons of all the energy states with magnetic moment parallel to the direction of the magnetic field.

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