Magnetic Susceptibility of Neutron Matter
- 22 December 1969
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 23 (25) , 1463-1466
- https://doi.org/10.1103/physrevlett.23.1463
Abstract
The magnetic susceptibility of a neutron gas at zero temperature, an idealization of neutron-star matter, is estimated for the realistic, soft-core nucleon-nucleon potential of Reid. For mass densities below twice that of ordinary nuclear matter, there is no sign of a ferromagnetically favorable instability of the normal ground state of the system, the effect of the interactions being to depress the magnetic susceptibility relative to its Fermi-gas value.Keywords
This publication has 28 references indexed in Scilit:
- The hard-sphere Fermi gas and ferromagnetism in neutron starsPhysics Letters A, 1969
- Effect of attractive nuclear forces on the onset of ferromagnetism in neutron star matterLettere al Nuovo Cimento (1971-1985), 1969
- Criteria for Ferromagnetism in Dense Neutron Fermi Liquids-Neutron StarsPhysical Review Letters, 1969
- Acceleration of High-Energy Cosmic Rays by PulsarsPhysical Review Letters, 1969
- Radio Emission From Magnetic Neutron Stars. A Possible Model for PulsarsPhysical Review Letters, 1969
- Ferromagnetic transition in superdense matter and neutron starsIl Nuovo Cimento B (1971-1996), 1969
- Proposed Test for the Radiation Mechanism of PulsarsNature, 1969
- Oblique Rotator and Pulsar RadiationNature, 1968
- Rotating Neutron Stars as the Origin of the Pulsating Radio SourcesNature, 1968
- Elements of the Brueckner-Goldstone Theory of Nuclear MatterReviews of Modern Physics, 1967