Neutrino emissivity and bulk viscosity of iso-CSL quark matter in neutron stars

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dc.creatorBlaschke, David B.
dc.creatorBerdermann, Jens
dc.date2007-10-27
dc.date.accessioned2026-07-07T10:57:42Z
dc.date.available2026-07-07T10:57:42Z
dc.descriptionWe present results for neutrino emissivities and bulk viscosities of a two-flavor color superconducting quark matter phase with isotropic color-spin-locked (iso-CSL) single-flavor pairing which fulfill the constraints on quark matter derived from cooling and rotational evolution of compact stars. We compare with results for the phenomenologically successful, but yet heuristic 2SC+X phase.
dc.description6 pages, 2 figures, to appear in the proceedings of QCD@Work 2007, Martina Franca (Italy)
dc.identifierhttps://arxiv.org/abs/0710.5243
dc.identifierhttp://arxiv.org/abs/0710.5243
dc.identifierAIPConf.Proc.964:290-295,2007
dc.identifierdoi:10.1063/1.2823866
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186843
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleNeutrino emissivity and bulk viscosity of iso-CSL quark matter in neutron stars
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