Collective modes of the order parameter in a triplet superfluid neutron liquid
arXiv:1206.3648 · doi:10.1103/PhysRevC.85.065502
Abstract
The complete spectrum of collective modes of the triplet order parameter in the superfluid neutron matter is examined in the BCS approximation below the pair-breaking threshold. The dispersion equations both for the unitary and nonunitary excitations are derived and solved in the limit of by taking into account the anisotropy of the energy gap for the case of -wave pairing. By our analysis, there is only one Goldstone mode which is associated with the broken gauge symmetry. We found no additional Goldstone modes associated with the broken rotational symmetry but found that the oscillations of the total angular momentum are qualitatively similar to the "normal-flapping" mode in the A-phase of superfluid Helium. There are also two collective modes associated with internal vibrations of the structure of the order parameter oscillating with and .
arXiv comment20 pages, 2 figures
References in corpus (16)
- Neutrino Energy Loss from the Plasma Process at all Temperatures and Densities
- Effects of Strong and Electromagnetic Correlations on Neutrino Interactions in Dense Matter
- Collective modes of asymmetric nuclear matter in Quantum HadroDynamics
- Neutrino emission from triplet pairing of neutrons in neutron stars
- Goldstone Bosons in the 3P2 Superfluid Phase of Neutron Matter and Neutrino Emission
- - Pairing in Dense Neutron Matter: The Spectrum of Solutions
- Neutrino emission due to Cooper pairing of nucleons in cooling neutron stars
- Superfluid Phase Transitions in Dense Neutron Matter
- Zero sound in triplet-correlated superfluid neutron matter
- Neutrino emission from spin waves in neutron spin-triplet superfluid
- Neutrino emissivity of - superfluid cores in neutron stars
- Superfluid phases of triplet pairing and neutrino emission from neutron stars
- New eigen-mode of spin oscillations in the triplet superfluid condensate in neutron stars
- Neutrino emission due to Cooper pairing of protons in cooling neutron stars: Collective effects
- Collective neutrino-pair emission due to Cooper pairing of protons in superconducting neutron stars
- Neutrino-pair emission due to electron-phonon scattering in a neutron star crust: a reappraisal
Cited by in corpus (24)
- Superfluidity in nuclear systems and neutron stars
- Viscosity of neutron star matter and -modes in rotating pulsars
- Superfluid phases of triplet pairing and rapid cooling of the neutron star in Cassiopeia A
- Magnetic Properties of Quantized Vortices in Neutron Superfluids in Neutron Stars
- Superfluids Are Topological
- Reexamining Ginzburg-Landau theory for neutron superfluidity in neutron stars
- The low lying modes of triplet-condensed neutron matter and their effective theory
- Neutrino emissivity of anisotropic neutron superfluids
- Phase structure of neutron superfluids in strong magnetic fields in neutron stars
- Collective excitations of a quantized vortex in superfluids in neutron stars
- Shear viscosity and the r-mode instability window in superfluid neutron stars
- Microscopic description of axisymmetric vortices in superfluids
- Massive and massless modes of the triplet phase of neutron matter
- Domain walls in neutron superfluids in neutron stars
- Critical endpoint and universality class of neutron superfluids in neutron stars
- Neutrino emissivity from Goldstone boson decay in magnetized neutron matter
- Coexistence phase of and superfluids in neutron stars
- Spin-polarized phases of superfluids in neutron stars
- Topological defects at the boundary of neutron superfluids in neutron stars
- Core structures of vortices in Ginzburg-Landau theory for neutron superfluids
- Proximity effects of vortices in neutron superfluids in neutron stars: Vortex core transitions and covalent bonding of vortex molecules
- Neutrino emission from Cooper pairs at finite temperatures
- Symmetry classification of uniform states in spin-2 Bose-Einstein condensates and neutron superfluids
- Emergent chirality and superfluidity of parity-doubled baryons in neutron stars