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Shear viscosity in a CFL quark star
Author(s) -
Cristina Manuel,
Antonio Dobado,
Felipe J. Llanes–Estrada
Publication year - 2005
Publication title -
journal of high energy physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.998
H-Index - 261
eISSN - 1126-6708
pISSN - 1029-8479
DOI - 10.1088/1126-6708/2005/09/076
Subject(s) - physics , mean free path , superfluidity , strange matter , quark–gluon plasma , boltzmann equation , phonon , scattering , quark , volume viscosity , condensed matter physics , qcd matter , viscosity , quantum mechanics
We compute the mean free path and shear viscosity in the color-flavor locked(CFL) phase of dense quark matter at low temperature T, when the contributionsof mesons, quarks and gluons to the transport coefficients are Boltzmannsuppressed. CFL quark matter displays superfluid properties, and transportphenomena in such cold regime are dominated by phonon-phonon scattering. Westudy superfluid phonons within thermal field theory and compute the mean freepath associated to their most relevant collision processes. Small-angleprocesses turn out to be more efficient in slowing transport phenomena in theCFL matter, while the mean free path relevant for the shear viscosity is lesssensitive to collinear scattering due to the presence of zero modes in theBoltzmann equation. In analogy with superfluid He4, we find the same T powerlaw for the superfluid phonon damping rate and mean free path. Our results arerelevant for the study of rotational properties of compact stars, and correctwrong estimates existing in the literature.Comment: 22 pages, 3 figures; it matches the published versio

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