Temperature dependence of magnetic susceptibility of nuclear matter: lowest order constrained variational calculations

Abstract

In this paper we study the magnetic susceptibility and other thermodynamic properties of the polarized nuclear matter at finite temperature using the lowest order constrained variational (LOCV) method employing the $A{V}_{18}$ potential. Our results show a monotonic behavior for the magnetic susceptibility which indicates that the spontaneous transition to the ferromagnetic phase does not occur for this system.

arXiv comment20 pages, 8 figures Phys. Rev C (2009) in press

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Cited by in corpus (16)

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• Maximum Mass of the Hot Neutron Star with the Quark Core
• Contraction of cold neutron star due to in the presence a quark core
• Finite temperature calculations for the spin polarized asymmetric nuclear matter with the LOCV method
• Magnetized hot neutron matter: lowest order constrained variational calculations
• Saturation properties of nuclear matter in the presence of strong magnetic field
• Hot Spin Polarized Strange Quark Stars in the Presence of Magnetic Field using a density dependent bag constant
• Influence of spin polarizability on liquid gas phase transition in the nuclear matter
• Neutron star calculations with the phenomenological three-nucleon force
• Nuclear matter calculations with the phenomenological three-nucleon interaction
• Hot magnetized nuclear matter: Thermodynamic and Saturation Properties
• Ferromagnetism of electron gas
• Calculation of the Structure Properties of Asymmetrical Nuclear Matter
• New Skyrme parametrizations to describe finite nuclei and neutron star matter with realistic effective masses. II. Adjusting the spin-dependent terms