Bulk viscosity in nuclear and quark matter: A short review

Abstract

The history and recent progresses in the study of bulk viscosity in nuclear and quark matter are reviewed. The constraints from baryon number conservation and electric neutrality in quark matter on particle densities and fluid velocity divergences are discussed.

A section is added to discuss the constraints from baryon number conservation and charge neutrality in bulk viscosity

References in corpus (5)

• Neutrino emission from compact stars and inhomogeneous color superconductivity
• Effect of hyperon-hyperon interaction on bulk viscosity and r-mode instability in neutron stars
• Phase space and quark mass effects in neutrino emissions in a color superconductor
• Baryon number conservation and enforced electric charge neutrality for bulk viscosity in quark matter
• Some issues about neutrino processes in color superconducting quark matter

Cited by in corpus (12)

• Stellar models with like--Tolman IV complexity factor
• Large amplitude behavior of the bulk viscosity of dense matter
• Gravitational cracking and complexity in the framework of gravitational decoupling
• Bulk viscosity in kaon-condensed color-flavor locked quark matter
• Bulk viscosity of superfluid hyperon stars
• Bulk viscosity from Urca processes: $npe\mu$ matter in the neutrino-trapped regime
• Bulk Viscosity of Relativistic $npe\mu$ Matter in Neutron-Star Mergers
• Temperature effects in pulsating superfluid neutron stars
• Leptonic contribution to the bulk viscosity of nuclear matter
• Hyperon bulk viscosity in strong magnetic fields
• Gravitational Cracking of General Relativistic Polytropes: a generalized scheme
• Double relativistic master polytrope for anisotropic matter