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Absence of two-flavor color-superconductivity in compact stars

Mark Alford1 and Krishna Rajagopal2

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The simplest pattern of color superconductivity involves BCS pairing between up and down quarks. We argue that this `2SC' phase will not arise within a compact star. A macroscopic volume of quark matter must be electrically neutral and must be a color singlet. Satisfying these requirements imposes a significant free energy cost on the 2SC phase, but not on color-flavor locked (CFL) quark matter, in which up, down and strange quarks all pair. As a function of increasing density, therefore, one may see a single phase transition from hadronic matter directly to CFL quark matter. Alternatively, there may be an intervening phase in which the different flavors self-pair, or pair with each other in a non-BCS pattern, such as in a crystalline color superconductor.


Keywords

Related Astrophysics (Neutron Stars, Supernovae etc.)

QCD

 

E-print Number: hep-ph/0204001

Cited: by |

Refers: to

PACS

12.38.-t Quantum chromodynamics

97.60.Bw Supernovae

12.39.-x Phenomenological quark models

97.60.Jd Neutron stars

Subjects

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 06 (June 2002)

Received 10 June 2002, accepted for publication 12 June 2002

Published 1 July 2002



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