2000/04/12 by I. Vidaña, Isaac Vidaña, A. Polls +5 · 4 citations
Earth and Planetary Sciences · Physics and Astronomy · #Atomic and Subatomic Physics Research #High-pressure geophysics and materials #Pulsars and Gravitational Waves Research #nucl-th
paper · pdf · doi:10.1103/physrevc.62.035801
published as Phys.Rev. C62 (2000) 035801 · 27 pages, LateX, includes 8 PostScript figures, (submitted to PRC)
arxiv created 2000/04/12 · openalex publication_date 2000/07/27 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
We present results from Brueckner-Hartree-Fock calculations for \ensuremathβ-stable neutron star matter with nucleonic and hyperonic degrees of freedom, employing the most recent parametrizations of the baryon-baryon interaction of the Nijmegen group. It is found that the only strange baryons emerging in \ensuremathβ-stable matter up to total baryonic densities of 1.2 fm^\ensuremath-3 are \ensuremathΣ^\ensuremath- and \ensuremathΛ. The corresponding equations of state are then used to compute properties of neutron stars such as masses and radii.