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Color Superconductivity and Blinking Proto-Neutron Stars

G. W. Carter
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Abstract

If quark matter exists in the cores of neutron stars, it is most likely color superconducting. Thus a phase transition from free to paired quark matter might occur during the first minute of proto-neutron star evolution. In this talk I discuss how critical behavior of the medium will modify neutrino diffusion, possibly leading to a short temporal variation in the neutrino signal detected on Earth.

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G. W. Carter. 2001-11-27. Color Superconductivity and Blinking Proto-Neutron Stars. https://arxiv.org/abs/hep-ph/0111353

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