Zero sound in triplet-correlated superfluid neutron matter
arXiv:1007.2803 · doi:10.1103/PhysRevC.83.055803
Abstract
The linear response of a superfluid neutron liquid onto external vector field is studied for the case of pairing. The consideration is limited to the case when the wave-length of the perturbation is large as compared to the coherence length in the superfluid matter and the transferred energy is small in comparison with the gap amplitude. The obtained results are used to analyse the collisionless phonon-like excitations of the condensate of superfluid neutrons. In particular, we analyze the case of neutron condensation into the state with which is conventionally considered as the preferable one in the bulk matter of neutron stars. Zero sound (if it exists) is found to be anisotropic and undergoes strong decrement below some temperature threshold depending substantially on the intensity of Fermi-liquid interactions.
16 pages, 2 figures
References in corpus (17)
- Pairing in nuclear systems: from neutron stars to finite nuclei
- Effective Nucleon Masses in Symmetric and Asymmetric Nuclear Matter
- Vector current conservation and neutrino emission from singlet-paired baryons in neutron stars
- Superfluid Heat Conduction and the Cooling of Magnetized Neutron Stars
- Triplet pairing in beta-stable neutron star matter
- 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
- Triplet Pairing in Neutron Matter
- Transport Theoretical Approach to the Nucleon Spectral Function in Nuclear Matter
- BCS approximation to the effective vector vertex of superfluid fermions
- Neutrino emission from spin waves in neutron spin-triplet superfluid
- Superfluid phases of triplet pairing and neutrino emission from neutron stars
- Short-Range Correlations in Nuclear Matter at Finite Temperatures and High Densities
- Transport equations and linear response of superfluid Fermi mixtures in neutron stars
- Short Range Correlations and Spectral Functions in Asymmetric Nuclear Matter
- Collective neutrino-pair emission due to Cooper pairing of protons in superconducting neutron stars
Cited by in corpus (20)
- Superfluidity in nuclear systems and neutron stars
- Magnetic Properties of Quantized Vortices in Neutron Superfluids in Neutron Stars
- Collective modes of the order parameter in a triplet superfluid neutron liquid
- Reexamining Ginzburg-Landau theory for neutron superfluidity in neutron stars
- Neutrino emissivity of anisotropic neutron superfluids
- Phase structure of neutron superfluids in strong magnetic fields in neutron stars
- Shear viscosity and the r-mode instability window in superfluid neutron stars
- Collective excitations of a quantized vortex in superfluids in neutron stars
- Microscopic description of axisymmetric vortices in superfluids
- Thermal conductivity due to phonons in the core of superfluid neutron stars
- Domain walls in neutron superfluids in neutron stars
- Critical endpoint and universality class of neutron superfluids in neutron stars
- 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
- Strongly interacting matter in extreme magnetic fields
- 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