Spin Polarized Asymmetric Nuclear Matter and Neutron Star Matter Within the Lowest Order Constrained Variational Method

Abstract

In this paper, we calculate properties of the spin polarized asymmetrical nuclear matter and neutron star matter, using the lowest order constrained variational (LOCV) method with the $A{V}_{18}$, $Reid93$, $U{V}_{14}$ and $A{V}_{14}$ potentials. According to our results, the spontaneous phase transition to a ferromagnetic state in the asymmetrical nuclear matter as well as neutron star matter do not occur.

21 pages, 11 figures

References in corpus (13)

• An accurate nucleon-nucleon potential with charge-independence breaking
• The equation of state for nucleon matter and neutron star structure
• Construction of high-quality Nucleon-Nucleon potential models
• Spin susceptibility of neutron matter at zero temperature
• Equation of state and magnetic susceptibility of spin polarized isospin asymmetric nuclear matter
• Modern nucleon-nucleon potentials and symmetry energy in infinite matter
• Spin polarized neutron matte and magnetic susceptibility within the Brueckner-Hartree-Fock approximation
• Ferromagnetic instabilities in neutron matter at finite temperature with the Skyrme interaction
• Spin polarized states in strongly asymmetric nuclear matter
• Neutrino propagation and spin zero sound in hot neutron matter with Skyrme interactions
• Landau parameters of nuclear matter in the spin and spin-isospin channels
• Polarized Neutron Matter: A Lowest Order Constrained Variational Approach
• Lowest Order Constrained Variational Calculation of the Polarized Nuclear Matter with the Modern $A{V}_{18}$ Potential

Cited by in corpus (36)

• Skyrme Interaction and Nuclear Matter Constraints
• Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XI: Stabilizing neutron stars against a ferromagnetic collapse
• Spin and spin-isospin instabilities in asymmetric nuclear matter at zero and finite temperatures using Skyrme functionals
• Extended Skyrme interactions for nuclear matter, finite nuclei and neutron stars
• Ferromagnetic neutron stars: axial anomaly, dense neutron matter, and pionic wall
• Nuclear response for the Skyrme effective interaction with zero range tensor terms
• Nuclear response for the Skyrme effective interaction with zero-range tensor terms. II. Sum rules and instabilities
• Nuclear response for the Skyrme effective interaction with zero-range tensor terms. III. Neutron matter and neutrino propagation
• Magnetization of neutron star matter
• Lowest order constrained variational calculation of polarized neutron matter at finite temperature
• Temperature dependence of magnetic susceptibility of nuclear matter: lowest order constrained variational calculations
• Calculation of the Structure Properties of a Strange Quark Star in the Presence of Strong Magnetic Field Using a Density Dependent Bag Constant
• Reexamining Ginzburg-Landau theory for neutron ${}^3{P}_2$ superfluidity in neutron stars
• Neutron Fermi Liquids under the presence of a strong magnetic field with effective nuclear forces
• Investigation of the field-induced ferromagnetic phase transition in spin polarized neutron matter: a lowest order constrained variational approach
• Neutron stars in Einstein-$\Lambda$ gravity: the cosmological constant effects
• Maximum Mass of the Hot Neutron Star with the Quark Core
• Phase structure of neutron ${}^3{P}_2$ superfluids in strong magnetic fields in neutron stars
• To which densities is spin-polarized neutron matter a weakly interacting Fermi gas?
• Domain walls in neutron ${}^3{P}_2$ superfluids in neutron stars
• Influence of strong magnetic field on the structure properties of strange quark stars
• Critical endpoint and universality class of neutron ${}^3{P}_2$ superfluids in neutron stars
• Finite temperature calculations for the spin polarized asymmetric nuclear matter with the LOCV method
• Magnetized hot neutron matter: lowest order constrained variational calculations
• Possibility of ferromagnetic neutron matter
• Coexistence phase of ${}^1{S}_0$ and ${}^3{P}_2$ superfluids in neutron stars
• Topological defects at the boundary of neutron ${}^3{P}_2$ superfluids in neutron stars
• LOCV calculations for polarized liquid ${}^{3}He$ with the spin-dependent correlation
• Hot Spin Polarized Strange Quark Stars in the Presence of Magnetic Field using a density dependent bag constant
• Nuclear matter calculations with the phenomenological three-nucleon interaction
• Neutron star calculations with the phenomenological three-nucleon force
• Hot magnetized nuclear matter: Thermodynamic and Saturation Properties
• Impact of choices for center-of-mass correction energy on the surface energy of Skyrme energy density functionals
• Three-body Force Effects on the Properties of Neutron-rich Nuclear Matter
• Calculation of the Structure Properties of Asymmetrical Nuclear Matter
• The effect of three-body nucleon-nucleon interaction on the ground state binding energy of the light nuclei