vix.ing · top · new · best · stats · spec

Finite-temperature calculations for spin-polarized asymmetric nuclear matter with the lowest order constrained variational method

2010/08/21 by M. Bigdeli, G. H. Bordbar, A. Poostforush
Chemistry · Physics and Astronomy · #Asymmetry #Atomic physics #Chemistry #Cold Atom Physics and Bose-Einstein Condensates #Condensed matter physics #Equation of state #Isospin #Nuclear matter #Nuclear physics research studies #Nucleon #Physics #Polarization (electrochemistry) #Quantum electrodynamics #Quantum mechanics #Quantum, superfluid, helium dynamics #Spin (aerodynamics) #Spin polarization #Symmetry (geometry) #Thermodynamics #Variational method #astro-ph.SR #nucl-th

paper · pdf · doi:10.1103/physrevc.82.034309

published as Phys.Rev.C82:034309,2010 · 18 pages, 7 figures Phys. Rev. C (2010) in press

arxiv created 2010/08/21 · openalex publication_date 2010/09/10 · arxiv updated 2014/11/21 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

The lowest order constrained variational technique has been used to investigate some of the thermodynamic properties of spin-polarized hot asymmetric nuclear matter, such as the free energy, symmetry energy, susceptibility, and equation of state. We have shown that the symmetry energy of the nuclear matter is substantially sensitive to the value of spin polarization. Our calculations show that the equation of state of the polarized hot asymmetric nuclear matter is stiffer for higher values of the polarization as well as the isospin asymmetry parameter. Our results for the free energy and susceptibility show that spontaneous ferromagnetic phase transition cannot occur for hot asymmetric matter.

Citations