Intrinsic magnetic polarizability contribution to the susceptibility of dense neutron matter

Details Intrinsic magnetic polarizability contribution to the susceptibility of dense neutron matter Intrinsic magnetic polarizability contribution to the susceptibility of dense neutron matter

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apl....16...57b&link_type=abstract

Astrophysical Letters, vol. 16, no. 2, 1975, p. 57-59.

Astronomy and Astrophysics

Astrophysics

2

Density Measurement, Magnetic Permeability, Neutron Stars, Stellar Magnetic Fields, Compton Effect, Magnetic Dipoles, Polarization Characteristics, Rayleigh Scattering

Scientific paper

It is shown that, apart from the neutron interaction contribution to the susceptibility of neutron stars, there is an additional contribution coming from the magnetic polarizability of individual neutrons. For magnetic polarizability approximately equal to 0.001 cu fm, this part overwhelms the interaction contribution for momentum of the corresponding Fermi gas at least about 3.5 per fm. No transition to ferromagnetic state is predicted in the density region of interest.

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