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Comparing neutron star predictions by various microscopic models
- Publication Year :
- 2009
-
Abstract
- We calculate several neutron star properties, for static and/or rotating stars, using equations of state based on different microscopic models. These include our Dirac-Brueckner-Hartree-Fock model and others derived from the non-relativistic Brueckner-Hartree-Fock approach implemented with microscopic three-body forces. The model dependence is discussed.<br />Comment: 8 pages, 8 figures, revtex4
- Subjects :
- Nuclear Theory
Subjects
Details
- Database :
- arXiv
- Publication Type :
- Report
- Accession number :
- edsarx.0906.0320
- Document Type :
- Working Paper