Equation of state and magnetic susceptibility of spin polarized isospin asymmetric nuclear matter
Creators
- 1. Dipartimento di Fisica 'E. Fermi', Universita di Pisa and INFN Sezione di Pisa, Via Buonarroti 2, I-56127 Pisa (Italy)
Description
Properties of spin-polarized isospin asymmetric nuclear matter are studied within the framework of the Brueckner-Hartree-Fock formalism. The single-particle potentials of neutrons and protons with spin up and down are determined for several values of the neutron and proton spin polarizations and the asymmetry parameter. It is found that the single-particle potentials exhibit an almost linear and symmetric variation as a function of these parameters. An analytic parametrization of the total energy per particle as a function of the asymmetry and spin polarizations is constructed. This parametrization is employed to compute the magnetic susceptibility of nuclear matter for several values of the asymmetry from neutron to symmetric matter. The results show no indication of a ferromagnetic transition at any density for any asymmetry of nuclear matter
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.66.045801;
- arXiv
- arXiv:nucl-th/0203061v1;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 66
- Journal Issue
- 4
- Journal Page Range
- p. 045801-045801.11
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36012704
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- ASYMMETRY; EQUATIONS OF STATE; HARTREE-FOCK METHOD; ISOSPIN; MAGNETIC SUSCEPTIBILITY; NEUTRONS; NUCLEAR MATTER; POLARIZATION; POTENTIALS; PROTONS; PULSARS; SPIN; SPIN ORIENTATION
- Descriptors DEC
- ANGULAR MOMENTUM; BARYONS; CALCULATION METHODS; COSMIC RADIO SOURCES; ELEMENTARY PARTICLES; EQUATIONS; FERMIONS; HADRONS; MAGNETIC PROPERTIES; MATTER; NUCLEONS; ORIENTATION; PARTICLE PROPERTIES; PHYSICAL PROPERTIES
Optional Information
- Notes
- (c) 2002 The American Physical Society