Friday, November 18, 2016, 2:00 pm — Small Seminar Room, Bldg. 510
In the first part of the talk I will discuss recent computations of the transport coefficients of dense QCD from the Kubo formalism on the basis of a two-flavor model of QCD. The second part of the talk will discuss the properties of compact stars featuring color superconducting phases of dense QCD. This will include modeling of massive compact stars, neutrino cooling of such stars, and possible signatures of a phase transition within the QCD phase diagram in the X-ray data from the young neutron star in Cassiopea A.
Hosted by: Heikki Mantysaari
11885 | INT/EXT | Events Calendar
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