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Related papers: Shear Viscosity in a CFL Quark Star

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Transport coefficients of dense quark matter are needed to study properties of compact stars. They can tell us about the cooling, vibrational and rotational properties of the star. We report below a computation of the shear viscosity in the…

High Energy Physics - Phenomenology · Physics 2017-08-23 Cristina Manuel

We compute one of the bulk viscosity coefficients of cold CFL quark matter in the temperature regime where the contribution of mesons, quarks and gluons to transport phenomena is Boltzmann suppressed. In that regime dissipation occurs due…

High Energy Physics - Phenomenology · Physics 2008-11-26 Cristina Manuel , Felipe Llanes-Estrada

At asymptotic high density and low temperature quarks form Cooper pairs in a color-flavor locked (CFL) configuration. The diquark condensates break spontaneously the baryon symmetry, and this fact makes the CFL phase also superfluid. At low…

High Energy Physics - Phenomenology · Physics 2009-06-25 Cristina Manuel

We calculate the kaonic contribution to the shear viscosity of quark matter in the kaon-condensed color-flavor locked phase (CFL-K0). This contribution comes from a light pseudo-Goldstone boson which arises from the spontaneous breaking of…

Nuclear Theory · Physics 2010-11-22 Mark G. Alford , Matt Braby , Simin Mahmoodifar

Thermal emission rates and mean free paths of photons in a color-flavor locked (CFL) phase of quark matter at high densities and moderate temperatures are evaluated. Our calculations are based on a low-energy effective theory for CFL matter…

High Energy Physics - Phenomenology · Physics 2009-11-10 C. Vogt , R. Rapp , R. Ouyed

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…

High Energy Physics - Phenomenology · Physics 2010-04-29 Matt Braby , Jingyi Chao , Thomas Schaefer

Color-flavor locked (CFL) quark matter at high densities is a color superconductor, which spontaneously breaks baryon number and chiral symmetry. Its low-energy thermodynamic and transport properties are therefore dominated by the H…

Nuclear Theory · Physics 2008-11-26 Mark G. Alford , Matt Braby , Andreas Schmitt

The bulk viscosities of two color-superconducting phases, the color-flavor locked (CFL) phase and the 2SC phase, are computed and compared to the result for unpaired quark matter. In the case of the CFL phase, processes involving kaons and…

Nuclear Theory · Physics 2008-11-26 Mark G. Alford , Andreas Schmitt

We evaluate the three bulk viscosity coefficients $\zeta_1, \zeta_2$ and $\zeta_3$ in the color-flavor locked (CFL) superfluid phase due to phonons and kaons, which are the lightest modes in that system. We first show that the computation…

High Energy Physics - Phenomenology · Physics 2011-08-08 Robert Bierkandt , Cristina Manuel

We present some results about dissipative processes in fermionic superfluids that are relevant for compact stars. At sufficiently low temperatures the transport properties of a superfluid are dominated by phonons. We report the values of…

High Energy Physics - Phenomenology · Physics 2011-02-01 M. Mannarelli , G. Colucci , C. Manuel

We calculate the bulk viscosity of color-superconducting quark matter in the color-flavor-locked (CFL) phase. We assume that the lightest bosons are the superfluid mode H and the kaons K0 and K+, and that there is no kaon condensate. We…

Nuclear Theory · Physics 2008-11-26 Mark G. Alford , Matt Braby , Sanjay Reddy , Thomas Schaefer

This thesis is devoted to properties of quark matter at high density and (comparatively) low temperature, which might exist in the interior of compact stars. The specific heat and the quark self energy in normal quark matter are discussed…

High Energy Physics - Phenomenology · Physics 2007-05-23 Andreas Gerhold

Matter at high density and low temperature is expected to be a color superconductor, which is a degenerate Fermi gas of quarks with a condensate of Cooper pairs near the Fermi surface that induces color Meissner effects. At the highest…

High Energy Physics - Phenomenology · Physics 2008-12-18 Mark G. Alford , Krishna Rajagopal , Thomas Schaefer , Andreas Schmitt

We study the shear and bulk viscosity coefficients as well as the thermal conductivity as arising from the collisions among phonons in superfluid neutron stars. We use effective field theory techniques to extract the allowed phonon…

Solar and Stellar Astrophysics · Physics 2014-12-01 Laura Tolos , Cristina Manuel , Sreemoyee Sarkar , Jaume Tarrus

We present the first calculation of the shear viscosity for two-flavor plane wave (FF) color superconducting quark matter. This is a member of the family of crystalline color superconducting phases of dense quark matter that may be present…

High Energy Physics - Phenomenology · Physics 2017-12-06 Sreemoyee Sarkar , Rishi Sharma

We review the effective field theory associated with the superfluid phonons that we use for the study of transport properties in the core of superfluid neutrons stars in their low temperature regime. We then discuss the shear and bulk…

Nuclear Theory · Physics 2021-03-08 Cristina Manuel , Laura Tolos

Some results about dissipative processes in superfluids are presented. We focus on fermionic superfluidity and restrict our analysis to the contribution of phonons to bulk viscosity, shear viscosity and thermal conductivity. At sufficiently…

High Energy Physics - Phenomenology · Physics 2010-11-02 Massimo Mannarelli , Cristina Manuel

We consider the phonon contribution to the bulk viscosities $\zeta_1, \zeta_2$ and $\zeta_3$ of a cold relativistic superfluid. We assume the low temperature $T$ regime and that the transport properties of the system are dominated by the…

High Energy Physics - Phenomenology · Physics 2010-04-06 Massimo Mannarelli , Cristina Manuel

We study the weak interaction rates involving Goldstone bosons in the Color Flavor Locked (CFL) quark matter. Neutrino mean free path and the rate of energy loss due to neutrino emission in a thermal plasma of CFL pions and kaons is…

Nuclear Theory · Physics 2008-11-26 Sanjay Reddy , Mariusz Sadzikowski , Motoi Tachibana

Dissipative processes acting in rotating neutron stars are essential in preventing the growth of the r-mode instability. We estimate the damping time of r-modes of an hypothetical compact quark star made up by color flavor locked quark…

High Energy Physics - Phenomenology · Physics 2009-01-09 Massimo Mannarelli , Cristina Manuel , Basil A. Sa'd
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