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Superfluidity of $Σ^-$ hyperons in $β$-stable neutron star matter

Isaac Vidana·Laura Tolos
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Abstract

In this work we evaluate the $^1S_0$ energy gap of $Σ^-$ hyperons in $β$-stable neutron star matter. We solve the BCS gap equation for an effective $Σ^-Σ^-$ pairing interaction derived from the most recent parametrization of the hyperon-hyperon interaction constructed by the Nijmegen group. We find that the $Σ^-$ hyperons are in a $^1S_0$ superfluid state in the density region $\sim 0.27-0.7$ fm$^{-3}$, with a maximum energy gap of order 8 MeV at a total baryon number density of $\sim 0.37$ fm$^{-3}$ and a $Σ^-$ fraction of about 8%. We examine the implications on neutron star cooling.

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Isaac Vidana, Laura Tolos. 2004-07-14. Superfluidity of $Σ^-$ hyperons in $β$-stable neutron star matter. https://doi.org/10.1103/physrevc.70.028802

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