Exploring the QCD phase diagram with compact stars

被引:12
作者
Blaschke, D
Grigorian, H [1 ]
Khalatyan, A
Voskresensky, DN
机构
[1] Univ Bielefeld, Fak Phys, D-33615 Bielefeld, Germany
[2] Joint Inst Nucl Res, Bogoliubov Lab Theoret Phys, Dubna 141980, Russia
[3] Univ Rostock, Fachbereich Phys, D-18051 Rostock, Germany
[4] Astrophys Inst Potsdam, D-14482 Potsdam, Germany
[5] Gesell Schwerionenforsch mbH, D-64291 Darmstadt, Germany
[6] Moscow Inst Phys & Engn, Moscow 115409, Russia
关键词
D O I
10.1016/j.nuclphysbps.2004.12.021
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We investigate a nonlocal chiral quark model with separable 4-fermion interaction for the case of U(3) flavor symmetry, and show that strange quark matter is unlikely to occur in a large enough volume of a compact star to entail remarkable observational consequences. The phase diagram in the two-flavor sector of such model has a critical end point of the line of first order chiral/deconfinement phase transitions on which a triple point marks the junction with the critical line for second order phase transitions to two-flavor color superconductivity (2SC below T similar to 80 MeV. Stable hybrid star configurations with large quark matter core in a color superconducting phase can exist. A consistent cooling phenomenology requires that all quark species be gapped, the minimal pairing gap of the order of 10 - 100 keV.
引用
收藏
页码:137 / 142
页数:6
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