Lambda hyperons equilibrate rapidly in post-collapse proto-neutron stars through nonleptonic NN to N Lambda processes and enhance low-energy muon neutrino opacities beyond nucleonic contributions.
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Diquark coupling in the NJL model is fixed near 1.5 times the scalar coupling and vector coupling below 1.1 times, yielding crossover equations of state that raise maximum neutron star masses and produce distinct radial oscillation frequencies potentially detectable as quark-matter signatures.
citing papers explorer
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$\Lambda$ hyperons in core-collapse supernovae: Equilibration and neutrino opacities
Lambda hyperons equilibrate rapidly in post-collapse proto-neutron stars through nonleptonic NN to N Lambda processes and enhance low-energy muon neutrino opacities beyond nucleonic contributions.
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Crossover Equation of State Constrained by Astronomical Observations and pQCD
Diquark coupling in the NJL model is fixed near 1.5 times the scalar coupling and vector coupling below 1.1 times, yielding crossover equations of state that raise maximum neutron star masses and produce distinct radial oscillation frequencies potentially detectable as quark-matter signatures.