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 , Reid93, , and 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.
4 More- Received 9 September 2007
DOI:https://doi.org/10.1103/PhysRevC.77.015805
©2008 American Physical Society