Color superconducting quark matter in compact stars

Physics – High Energy Physics – High Energy Physics - Phenomenology

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Invited talk at the Conference on Compact Stars in the QCD Phase Diagram, Copenhagen, August 15-18, 2001. LaTeX with eps figs,

Scientific paper

When nuclear matter reaches a high enough density, we expect that the
nucleons will overlap so much as to lose their separate identities, and merge
into quark matter. In this talk I will review some theoretical expectations and
speculations about quark matter, focusing on the phenomenon of quark pair
condensation (color superconductivity) and its application to compact stars.

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