The relativistic entrainment matrix of a superfluid nucleon-hyperon mixture. II. Effect of finite temperatures
arXiv:0907.0010 · doi:10.1103/PhysRevC.80.015803
Abstract
We calculate the important quantity of superfluid hydrodynamics, the relativistic entrainment matrix for a nucleon-hyperon mixture at arbitrary temperature. In the nonrelativistic limit this matrix is also termed the Andreev-Bashkin or mass-density matrix. Our results can be useful for modeling the pulsations of massive neutron stars with superfluid nucleon-hyperon cores and for studies of the kinetic properties of superfluid baryon matter.
arXiv comment10 pages, 1 figure, accepted for publication in Phys. Rev. C
References in corpus (20)
- Theory of ultracold Fermi gases
- Color superconductivity in dense quark matter
- The Physics of Neutron Stars
- Specular Andreev reflection in graphene
- Neutrino Emission from Neutron Stars
- The Cooling of Compact Stars
- Cooling neutron stars and superfluidity in their interiors
- Thermal Conductivity of Neutrons in Neutron Star Cores
- Entrainment parameters in cold superfluid neutron star core
- A Relativistic Mean Field Model for Entrainment in General Relativistic Superfluid Neutron Stars
- S-wave Pairing of Hyperons in Dense Matter
- The entrainment matrix of a superfluid neutron-proton mixture at a finite temperature
- Temperature-dependent pulsations of superfluid neutron stars
- Occurrence of Hyperon Superfluidity in Neutron Star Cores
- The relativistic entrainment matrix of a superfluid nucleon-hyperon mixture at zero temperature
- Bulk viscosity of superfluid hyperon stars
- BCS and generalized BCS superconductivity in relativistic quantum field theory. I. formulation
- Damping of sound waves in superfluid nucleon-hyperon matter of neutron stars
- Superfluidity of hyperons in -stable neutron star matter
- BCS and Generalized BCS Superconductivity in Relativistic Quantum Field Theory. II. Numerical Calculations
Cited by in corpus (32)
- Equations of state for supernovae and compact stars
- Relativistic fluid dynamics: physics for many different scales
- Reaction rates and transport in neutron stars
- Modelling pulsar glitches with realistic pinning forces: a hydrodynamical approach
- Explaining observations of rapidly rotating neutron stars in LMXBs
- Physics input for modelling superfluid neutron stars with hyperon cores
- Superfluid hyperon bulk viscosity and the r-mode instability of rotating neutron stars
- Instability windows and evolution of rapidly rotating neutron stars
- Composition temperature-dependent g-modes in superfluid neutron stars
- The dynamics of dissipative multi-fluid neutron star cores
- Relativistic dynamics of superfluid-superconducting mixtures in the presence of topological defects and an electromagnetic field with application to neutron stars
- Evolution of the magnetic field in neutron stars
- Temperature effects in pulsating superfluid neutron stars
- Oscillations of superfluid hyperon stars: decoupling scheme and g-modes
- Quasi-normal modes of superfluid neutron stars
- Relativistic finite temperature multifluid hydrodynamics in a neutron star from a variational principle
- Dissipation in relativistic superfluid neutron stars
- Constraining neutron superfluidity with -mode physics
- Numerical models for stationary superfluid neutron stars in general relativity with realistic equations of state
- Decoupling of superfluid and normal modes in pulsating neutron stars
- Transport equations and linear response of superfluid Fermi mixtures in neutron stars
- Velocity-dependent energy gaps and dynamics of superfluid neutron stars
- Entrainment effects in neutron-proton mixtures within the nuclear-energy density functional theory. I. Low-temperature limit
- Temperature-dependent r-modes in superfluid neutron stars stratified by muons
- The entrainment matrix of a superfluid nucleon mixture at finite temperatures
- Entrainment effects in neutron-proton mixtures within the nuclear-energy density functional theory. II. Finite temperatures and arbitrary currents
- A minimal model for finite temperature superfluid dynamics
- Isospin dependence of entrainment in superfluid neutron stars in a relativistic model
- Temperature-dependent oscillation modes in rotating superfluid neutron stars
- Resonance suppression of the r-mode instability in superfluid neutron stars: Accounting for muons and entrainment
- Diffusion in superfluid Fermi mixtures: General formalism
- Dissipative superfluid relativistic magnetohydrodynamics of a multicomponent fluid: the combined effect of particle diffusion and vortices