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Prashanth Jaikumar McGill University Cold and dense quark matter exhibits BCS-type pairing with critical temperatures that make neutron stars, the likely candidates to support such matter in their cores, the hottest superconductors in the universe. I will discuss general aspects of color superconductivity followed by the neutrino signature from quark matter in neutron stars, and comment on the possibility of it's observation through neutrinos.
Tuesday, September 10th 2002, 12:15 |