Modified NJL model exploration finds viable parameter space where beta-equilibrated CFL quark matter is absolutely stable, supporting self-bound quark stars consistent with NICER, LIGO/Virgo, GW190814, and HESS J1731-347 observations.
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The stability of color-flavor-locked quark matter and massive CFL quark stars
Modified NJL model exploration finds viable parameter space where beta-equilibrated CFL quark matter is absolutely stable, supporting self-bound quark stars consistent with NICER, LIGO/Virgo, GW190814, and HESS J1731-347 observations.