1. The role of chiral symmetry restoration, deconfinement and color superconductivity for (rotating) compact star configurations
* SPEAKERS
Name
Affiliation
E-mail
Prof. David Blaschke, JINR
Russia and University of Rostock
* HOST(Applicant)
Name
Affiliation
E-mail
-
* DATE / TIME
2002-01-17, 9:30-12:00
* PLACE
Kyung Book National Univ. 제1과학관(물리학관 206호)
* ABSTRACT
An elementary introduction into the subject will be given. The new developments on which I want to focus do concern modeling of the high-density QCD phase in the vicinity of the deconfinement transition, where color superconductivity might occur. Consequences of such a phase transition for explosive phenomena (GRB, Supernovae, Hypernovae) have recently been discussed, e.g. by Sannino, Ouyed, Hsu, Hong and others. We have performed detailed calculations of cooling, magnetic fields and also of structure and stability of compact stars with (superconducting) quark matter cores.
