3PF2 pairing in high-density neutron matter

Abstract

The onset of the 3PF2 superfluid phase in high-density neutron matter is studied within the BCS framework with two and three body forces. Owing to the strong correlations the energy gap is so sizeably quenched as to demand to reconsider the role of superfluidity in neutron-star phenomena.

4 pages, 2 figures

References in corpus (18)

• Rapid Cooling of the Neutron Star in Cassiopeia A Triggered by Neutron Superfluidity in Dense Matter
• Cooling neutron star in the Cassiopeia~A supernova remnant: Evidence for superfluidity in the core
• Polarization contributions to the spin-dependence of the effective interaction in neutron matter
• Screening Effects in Superfluid Nuclear and Neutron Matter within Brueckner Theory
• BCS-BEC crossover of neutron pairs in symmetric and asymmetric nuclear matter
• Goldstone Bosons in the 3P2 Superfluid Phase of Neutron Matter and Neutrino Emission
• ${}^3{P}_2$-${}^3{F}_2$ Pairing in Dense Neutron Matter: The Spectrum of Solutions
• Three-body force effect on nucleon momentum distributions in asymmetric nuclear matter within the framework of the extended BHF approach
• Unified description of neutron superfluidity in the neutron-star crust with analogy to anisotropic multi-band BCS superconductors
• Constraining the nuclear pairing gap with pairing vibrations
• On the superfluid properties of the inner crust of neutron stars
• Relativistic description of BCS-BEC crossover in nuclear matter
• BCS-BEC Crossover in Symmetric Nuclear Matter at Finite Temperature: Pairing Fluctuation and Pseudogap
• Microscopic evaluation of the pairing gap
• BCS-BEC crossover in nuclear matter with the relativistic Hartree-Bogoliubov theory
• Neutrino emissivity of ${}^3{P}_2$-${}^3{F}_2$ superfluid cores in neutron stars
• Cooper pair sizes in superfluid nuclei in a simplified model
• Nuclear superfluidity in isospin asymmetric matter within the Skyrme model

Cited by in corpus (32)

• Neutron Stars and the Nuclear Equation of State
• Nucleon Effective Masses in Neutron-Rich Matter
• Superfluidity in nuclear systems and neutron stars
• Superfluidity and Superconductivity in Neutron Stars
• Pairing in high-density neutron matter including short- and long-range correlations
• Pairing in high-density neutron matter including short- and long-range correlations
• Upper bounds on r-mode amplitudes from observations of low-mass X-ray binary neutron stars
• Nuclear medium cooling scenario in the light of new Cas A cooling data and the 2 M_sun pulsar mass measurements
• Pairing in neutron matter: New uncertainty estimates and three-body forces
• Instability windows and evolution of rapidly rotating neutron stars
• Viscosity of neutron star matter and $r$-modes in rotating pulsars
• Nuclear pairing from microscopic forces: singlet channels and higher-partial waves
• Role of nucleonic Fermi surface depletion in neutron star cooling
• Pairing and short-range correlations in nuclear systems
• Triplet Pairing in pure neutron matter
• Anti-glitches within the standard scenario of pulsar glitches
• Could the low braking index pulsar PSR J1734-3333 evolve into a magnetar?
• Reinvestigation of the electron fraction and electron Fermi energy of neutron star
• Medium polarization in asymmetric nuclear matter
• Pairing in pure neutron matter
• Three-nucleon forces and superfluidity in neutron matter
• Medium polarization effects in 3SD1 spin-triplet pairing
• Neutron-proton pairing in Nuclear Matter
• Equation of state of superfluid neutron matter with low-momentum interactions
• Breakdown of the tensor component in the Skyrme energy density functional
• Neutron star cooling and mass distributions
• Vector-boson condensates, spin-triplet superfluidity of paired neutral and charged fermions, and $3P_2$ pairing of nucleons
• A local-density-approximation description of high-momentum tails in isospin asymmetric nuclei
• Effects of nucleon-nucleon short-range correlation and symmetry energy on the evolution of newly born magnetars
• Neutron star cooling with a dynamic stellar structure
• Single-Particle Spectrum of Pure Neutron Matter
• Coexistence of isospin I = 0 and I = 1 pairings in asymmetric nuclear matter