Spin polarized asymmetric nuclear matter and neutron star matter within the lowest order constrained variational method

G. H. Bordbar and M. Bigdeli
Phys. Rev. C 77, 015805 – Published 16 January 2008

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 AV18, Reid93, UV14, and AV14 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.

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  • Received 9 September 2007

DOI:https://doi.org/10.1103/PhysRevC.77.015805

©2008 American Physical Society

Authors & Affiliations

G. H. Bordbar1,2,* and M. Bigdeli1,3

  • 1Department of Physics, Shiraz University, Shiraz 71454, Iran
  • 2Research Institute for Astronomy and Astrophysics of Maragha, P. O. Box 55134-441, Maragha, Iran
  • 3Department of Physics, Zanjan University, Zanjan, Iran

  • *Corresponding author: bordbar@physics.susc.ac.ir

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Issue

Vol. 77, Iss. 1 — January 2008

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