skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Cooling of neutron stars with color superconducting quark cores

Journal Article · · Physical Review. C, Nuclear Physics
 [1];  [2];  [3]
  1. Institut fuer Physik, Universitaet Rostock, D-18051 Rostock (Germany)
  2. Fakultaet fuer Physik, Universitaet Bielefeld, D-33615 Bielefeld (Germany)
  3. Theory Division, GSI mbH, D-64291 Darmstadt (Germany)

We show that within a recently developed nonlocal, chiral quark model the critical density for a phase transition to color superconducting quark matter under neutron star conditions can be low enough for these phases to occur in compact star configurations with masses below 1.3 M{sub {center_dot}}. We study the cooling of these objects in isolation for different values of the gravitational mass. Our equation of state (EoS) allows for two-flavor color superconductivity (2SC) quark matter with a large quark gap ({approx}100 MeV) for u and d quarks of two colors that coexists with normal quark matter within a mixed phase in the hybrid star interior. We argue that, if the phases with unpaired quarks were allowed, the corresponding hybrid stars would cool too fast. If they occurred for M<1.3 M{sub {center_dot}}, as follows from our EoS, one could not appropriately describe the neutron star cooling data existing today. We discuss a ''2SC+X'' phase as a possibility for having all quarks paired in two-flavor quark matter under neutron star constraints, where the X gap is of the order of 10 keV-1 MeV. Density-independent gaps do not allow us to fit the cooling data. Only the presence of an X gap that decreases with increasing density would allow us to appropriately fit the data in a similar compact star mass interval to that following from a purely hadronic model. This scenario is suggested as an alternative explanation of the cooling data in the framework of a hybrid star model.

OSTI ID:
20696104
Journal Information:
Physical Review. C, Nuclear Physics, Vol. 71, Issue 4; Other Information: DOI: 10.1103/PhysRevC.71.045801; (c) 2005 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2813
Country of Publication:
United States
Language:
English

Similar Records

Single-flavor CSL phase in compact stars
Journal Article · Fri Aug 29 00:00:00 EDT 2008 · AIP Conference Proceedings · OSTI ID:20696104

Sequential deconfinement of quark flavors in neutron stars
Journal Article · Tue Dec 15 00:00:00 EST 2009 · Physical Review. C, Nuclear Physics · OSTI ID:20696104

Phase diagram of three-flavor quark matter under compact star constraints
Journal Article · Thu Sep 15 00:00:00 EDT 2005 · Physical Review. D, Particles Fields · OSTI ID:20696104