Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2009-09-23
Phys.Rev.C81:045205,2010
Physics
High Energy Physics
High Energy Physics - Phenomenology
20 pages, 4 figures - Changed small numerical error and added some comments based on discussions; conclusions unchanged
Scientific paper
10.1103/PhysRevC.81.045205
We compute the thermal conductivity of color-flavor locked (CFL) quark matter. At temperatures below the scale set by the gap in the quark spectrum, transport properties are determined by collective modes. In this work we focus on the contribution from the lightest modes, the superfluid phonon and the massive neutral kaon. The calculation is done in the framework of kinetic theory, using variational solutions of the linearized Boltzmann equation. We find that the thermal conductivity due to phonons is \kappa^P =1.04 10^{26} mu_{500}^8 \Delta_{50}^{-6} erg/(cm s K), where \mu_{500} is the chemical potential in units of 500 MeV and \Delta_{50} is the gap in units of 50 MeV. The contribution of kaons is \kappa^K = 2.81 10^{21} f_{\pi,100}^4 T_{MeV}^{1/2} m_{10}^{-5/2} erg/(cm s K), where f_{\pi,100} is the pion decay constant in units of 100 MeV, T_{MeV} is the temperature in units of 1 MeV, and m_{10} is the kaon mass in units of 10 MeV. These values are smaller than previous estimates, but still much larger than (in the case of phonons) or similar to (for kaons) the corresponding values in nuclear matter. From the phonon thermal conductivity we estimate that a CFL quark matter core of a compact star becomes isothermal on a timescale of a few seconds.
Braby Matt
Chao Jingyi
Schaefer Thomas
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