Abstract
We perform Brueckner-Hartree-Fock calculations of hypernuclear matter at finite temperature and provide convenient analytical parametrizations of the results. We then study the properties of (proto)neutron stars containing hyperons. We find important effects of trapping and finite temperature on the structure of hyperonic stars.
- Received 4 November 2010
DOI:https://doi.org/10.1103/PhysRevC.83.025804
©2011 American Physical Society
Synopsis
Hyperon stars
Published 3 March 2011
Dense matter containing strange quarks may significantly affect neutron star formation.
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