The extension of radiative viscosity to superfluid matter

Abstract

The radiative viscosity of superfluid $npe$ matter is studied, and it is found that to the lowest order of $\delta \mu /T$ the ratio of radiative viscosity to bulk viscosity is the same as that of the normal matter.

4 pages

References in corpus (9)

• Bulk viscosity of superfluid neutron stars
• Bulk viscosity of strange quark matter: Urca versus non-leptonic processes
• Bulk viscosity of spin-one color superconductors with two quark flavors
• Bulk viscosity of superfluid hyperon stars
• Bulk viscosity in nuclear and quark matter: A short review
• Non-equilibrium beta processes in superfluid neutron star cores
• Non-Equilibrium Beta Processes in Neutron Stars: A Relationship between the Net Reaction Rate and the Total Emissivity of Neutrinos
• Neutrino Emissivity of Non-equilibrium beta processes With Nucleon Superfluidity
• Radiative viscosity of neutron stars