Bulk viscosity of spin-one color superconducting strange quark matter

Journal Article · Fri Oct 15 04:00:00 EDT 2010 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.82.085007· OSTI ID:21432410

Xinyang, Wang ^[1]; Shovkovy, Igor A ^[1]

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1. Department of Physics, Arizona State University, Tempe, Arizona 85287 (United States)

The bulk viscosity in spin-one color superconducting strange quark matter is calculated by taking into account the interplay between the nonleptonic and semileptonic week processes. In agreement with previous studies, it is found that the inclusion of the semileptonic processes may result in non-negligible corrections to the bulk viscosity in a narrow window of temperatures. The effect is generally more pronounced for pulsars with longer periods. Compared to the normal phase, however, this effect due to the semileptonic processes is less pronounced in spin-one color superconductors. Assuming that the critical temperature of the phase transition is much larger than 40 keV, the main effect of spin-one color superconductivity in a wide range of temperatures is an overall increase of the bulk viscosity with respect to the normal phase. The corresponding enhancement factor reaches up to about 9 in the polar and A phases, about 25 in the planar phase, and about 29 in the color-spin-locked (CSL) phase. This factor is determined by the suppression of the nonleptonic rate in color superconducting matter and, therefore, may be even larger if all quark quasiparticles happen to be gapped.

• OSTI ID: 21432410
• Journal Information: Physical Review. D, Particles Fields, Journal Name: Physical Review. D, Particles Fields Journal Issue: 8 Vol. 82; ISSN PRVDAQ; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ANGULAR MOMENTUM
COLOR MODEL
COMPOSITE MODELS
COMPUTERIZED SIMULATION
CORRECTIONS
COSMIC RADIO SOURCES
CRITICAL TEMPERATURE
DECAY
ELECTRIC CONDUCTIVITY
ELECTRICAL PROPERTIES
ELEMENTARY PARTICLES
ENERGY RANGE
FERMIONS
KEV RANGE
KEV RANGE 10-100
MATHEMATICAL MODELS
MATTER
PARTICLE DECAY
PARTICLE MODELS
PARTICLE PROPERTIES
PHASE TRANSFORMATIONS
PHYSICAL PROPERTIES
PULSARS
QUARK MATTER
QUARK MODEL
QUARKS
QUASI PARTICLES
S QUARKS
SEMILEPTONIC DECAY
SIMULATION
SPIN
STRANGE PARTICLES
SUPERCONDUCTIVITY
THERMODYNAMIC PROPERTIES
TRANSITION TEMPERATURE
VISCOSITY
WEAK HADRONIC DECAY
WEAK PARTICLE DECAY