Alford MG, Nishimura H, Sedrakian A. Transport coefficients of two-flavor superconducting quark matter. Physical Review C. 2014;90(5): 055205.Background: The two-flavor color superconducting (2SC) phase of quark matter is a possible constituent of the core of neutron stars. To assess its impact on the observable behavior of the star one must analyze transport properties, which in 2SC matter are controlled by the scattering of gapless fermionic modes by each other and possibly also by color-magnetic flux tubes. Purpose: We determine the electrical and thermal conductivities and the shear viscosity of 2SC matter. Methods: We use a variational formulation of transport theory, treating the strong and electromagnetic interactions via a weak coup...
We pose two key questions about color superconductivity: What are the effects of the large strange q...
Color-flavor locked (CFL) quark matter expels color-magnetic fields due to the Meissner effect. One ...
Already more that 40 years ago, it has been suggested that because of the enormous mass densities in...
We have calculated different transport coefficients such as shear, bulk viscosities and electrical c...
We review the calculations of the kinetic coefficients (thermal conductivity, shear viscosity, momen...
We compute the transport coefficients, namely, the coefficients of shear and bulk viscosity, as well...
In this thesis, we study the thermodynamics of two-flavour colour superconductivity and the effects...
We study thermodynamic and transport properties for the isotropic color-spin-locking (iso-CSL) phas...
We compute the shear viscosity in the color-flavor locked (CFL) phase of dense quark matter at low t...
QCD with two light quark flavors at high baryonic density and low temperature is a color superconduc...
We consider the contribution of the Urca-type processes to the bulk viscosity of several spin-one co...
The transport properties of neutron star matter play an important role in many astrophysical process...
We review the effective field theory associated with the superfluid phonons that we use for the stud...
We review the effective field theory associated with the superfluid phonons that we use for the stud...
The bulk viscosity of three-flavor color-superconducting quark matter originating from the nonlepton...
We pose two key questions about color superconductivity: What are the effects of the large strange q...
Color-flavor locked (CFL) quark matter expels color-magnetic fields due to the Meissner effect. One ...
Already more that 40 years ago, it has been suggested that because of the enormous mass densities in...
We have calculated different transport coefficients such as shear, bulk viscosities and electrical c...
We review the calculations of the kinetic coefficients (thermal conductivity, shear viscosity, momen...
We compute the transport coefficients, namely, the coefficients of shear and bulk viscosity, as well...
In this thesis, we study the thermodynamics of two-flavour colour superconductivity and the effects...
We study thermodynamic and transport properties for the isotropic color-spin-locking (iso-CSL) phas...
We compute the shear viscosity in the color-flavor locked (CFL) phase of dense quark matter at low t...
QCD with two light quark flavors at high baryonic density and low temperature is a color superconduc...
We consider the contribution of the Urca-type processes to the bulk viscosity of several spin-one co...
The transport properties of neutron star matter play an important role in many astrophysical process...
We review the effective field theory associated with the superfluid phonons that we use for the stud...
We review the effective field theory associated with the superfluid phonons that we use for the stud...
The bulk viscosity of three-flavor color-superconducting quark matter originating from the nonlepton...
We pose two key questions about color superconductivity: What are the effects of the large strange q...
Color-flavor locked (CFL) quark matter expels color-magnetic fields due to the Meissner effect. One ...
Already more that 40 years ago, it has been suggested that because of the enormous mass densities in...