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Diffusion of Neutrinos in Proto-Neutron Star Matter with Quarks
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Neutrino opacities important in the evolution of a proto-neutron star containing quark matter are studied. The results for pure quark matter are compared with limiting expressions previously derived, and are generalized to the temperatures, neutrino degeneracies and lepton contents encountered in a proto-neutron star's evolution. We find that the appearance of quarks in baryonic matter drastically reduces the neutrino opacity for a given entropy, the reduction being sensitive to the thermodynamic conditions in the mixed quark-hadron phase.
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Cited by 2 Pith papers
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Neutrino absorption in two-flavor color-superconducting quark matter
In 2SC quark matter, neutrino absorption is dominated by strange-quark capture at low temperature, and a degenerate neutrino gas at electron lepton fraction 0.1 has a mean free path of meters or less.
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Self-consistent thermodynamical treatment for quark matter in quasi-particle model at finite temperature
A counterterm-free grand-canonical quasiparticle model gives quark star equations of state whose mass-radius and tidal deformability curves match current astronomical limits when vector repulsion is added.
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