Superfluidity of hyperons in -stable neutron star matter
arXiv:nucl-th/0405010 · doi:10.1103/PhysRevC.70.028802
Abstract
In this work we evaluate the energy gap of hyperons in -stable neutron star matter. We solve the BCS gap equation for an effective pairing interaction derived from the most recent parametrization of the hyperon-hyperon interaction constructed by the Nijmegen group. We find that the hyperons are in a superfluid state in the density region fm, with a maximum energy gap of order 8 MeV at a total baryon number density of fm and a fraction of about 8%. We examine the implications on neutron star cooling.
4 pages, double column, 4 figures. Accepted in PRC
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