Color Superconductivity and Blinking Proto-Neutron Stars

Details Color Superconductivity and Blinking Proto-Neutron Stars Color Superconductivity and Blinking Proto-Neutron Stars

2001-11-27

arxiv.org/abs/hep-ph/0111353v1

eConf C010815 (2002) 149-154

Physics

High Energy Physics

High Energy Physics - Phenomenology

6 pages, 4 figures, includes econfmacros.tex; talk at "Compact Stars in the QCD Phase Diagram", Nordita, 15-18 August 2001

Scientific paper

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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