Entrainment effects in neutron-proton mixtures within the nuclear-energy density functional theory. I. Low-temperature limit
arXiv:2102.02474 · doi:10.1103/PhysRevC.100.065801
Abstract
Mutual entrainment effects in cold neutron-proton mixtures are studied in the framework of the self-consistent nuclear energy-density functional theory. Exact expressions for the mass currents, valid for both homogeneous and inhomogeneous systems, are directly derived from the time-dependent Hartree-Fock equations with no further approximation. The equivalence with the Fermi-liquid expression is also demonstrated. Focusing on neutron-star cores, a convenient and simple analytical formulation of the entrainment matrix in terms of the isovector effective mass is found, thus allowing to relate entrainment phenomena in neutron stars to isovector giant dipole resonances in finite nuclei. Results obtained with different functionals are presented. These include the Brussels-Montreal functionals, for which unified equations of state of neutron stars have been recently calculated.
arXiv comment21 pages, 2 figures
References in corpus (39)
- Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII: Stiffness and stability of neutron-star matter
- Pairing in nuclear systems: from neutron stars to finite nuclei
- Rapid Cooling of the Neutron Star in Cassiopeia A Triggered by Neutron Superfluidity in Dense Matter
- Nuclear energy density optimization: Large deformations
- Cooling neutron star in the Cassiopeia~A supernova remnant: Evidence for superfluidity in the core
- Models of Pulsar Glitches
- Analytical representations of unified equations of state for neutron-star matter
- Neutron conduction in the inner crust of a neutron star in the framework of the band theory of solids
- Local Density Approximation for proton-neutron pairing correlations. I. Formalism
- Nucleon Effective Masses in Neutron-Rich Matter
- Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XI: Stabilizing neutron stars against a ferromagnetic collapse
- Time-odd components in the mean field of rotating superdeformed nuclei
- Heavy-ions collisions and fission dynamics with the time-dependent Hartree-Fock theory and its extensions
- From Brueckner Approach to Skyrme-type Energy Density Functional
- On the dynamics of superfluid neutron star cores
- Neutron Matter from Low to High Density
- Local nuclear energy density functional at next-to-next-to-next-to-leading order
- Properties of the nuclear medium
- Low-Energy Heavy-Ion Reactions and the Skyrme Effective Interaction
- Superfluidity and Superconductivity in Neutron Stars
- Self-interaction errors in nuclear energy density functionals
- Entrainment parameters in cold superfluid neutron star core
- A Relativistic Mean Field Model for Entrainment in General Relativistic Superfluid Neutron Stars
- The entrainment matrix of a superfluid neutron-proton mixture at a finite temperature
- Diffusive nuclear burning in cooling simulations and application to new temperature data of the Cassiopeia A neutron star
- Upper limits on the rapid cooling of the Central Compact Object in Cas A
- Finite amplitude method applied to giant dipole resonance in heavy rare-earth nuclei
- Extended Skyrme interactions for nuclear matter, finite nuclei and neutron stars
- Isospin splitting of nucleon effective mass from giant resonances in Pb
- The relativistic entrainment matrix of a superfluid nucleon-hyperon mixture at zero temperature
- Entrainment in Superfluid Neutron Star Crusts: Hydrodynamic Description and Microscopic Origin
- R-modes of neutron stars with the superfluid core
- The relativistic entrainment matrix of a superfluid nucleon-hyperon mixture. II. Effect of finite temperatures
- Nuclear dipole polarizability from mean-field modeling constrained by chiral effective field theory
- Numerical models for stationary superfluid neutron stars in general relativity with realistic equations of state
- The nucleon effective mass and its isovector splitting
- The entrainment matrix of a superfluid nucleon mixture at finite temperatures
- Isospin dependence of entrainment in superfluid neutron stars in a relativistic model
- Nonlinear approach to the entrainment matrix of superfluid nucleon mixture at zero temperature
Cited by in corpus (16)
- A superfluid perspective on neutron star dynamics
- Insights into the physics of neutron star interiors from pulsar glitches
- Time-dependent extension of the self-consistent band theory for neutron star matter: Anti-entrainment effects in the slab phase
- S pairing gaps, chemical potential and entrainment matrix in superfluid neutron-star cores for the Brussels-Montreal functionals
- Properties of a quantum vortex in neutron matter
- Entrainment effects in neutron-proton mixtures within the nuclear-energy density functional theory. II. Finite temperatures and arbitrary currents
- Superfluid density in linear response theory : pulsar glitches from the inner crust of neutron stars
- Gapless superfluidity in neutron stars: Thermal properties
- Gapless superfluidity in neutron stars: Normal-fluid fraction
- Superfluid fraction in the slab phase of the inner crust of neutron stars
- Superfluid fraction in the crystalline crust of a neutron star: role of BCS pairing
- Time-dependent nuclear energy-density functional theory toolkit for neutron star crust: Dynamics of a nucleus in a neutron superfluid
- Diffusion in superfluid Fermi mixtures: General formalism
- Vortex pinning in the superfluid core of relativistic neutron stars
- Roton instabilities in the superfluid outer core of neutron stars
- Superfluid fraction in the crystalline crust of a neutron star: role of quantum zero-point motion of ions