Magnetic Properties of Quantized Vortices in Neutron Superfluids in Neutron Stars
arXiv:1512.01946 · doi:10.1103/PhysRevC.93.035804
Abstract
We discuss quantized vortices in neutron superfluids, which are believed to realize in high density neutron matter such as neutron stars. By using the Ginzburg-Landau free energy for superfluids, we determine the ground state in the absence and presence of the external magnetic field, and numerically construct quantized vortices in the absence and presence of the external magnetic field along the vortex axis (poloidal) or angular direction (toroidal). We find in certain situations the spontaneous magnetization of the vortex core, whose typical magnitude is about Gauss, but the net magnetic field in a neutron star is negligible because of the ratio of the vortex core size fm and the intervortex distance m in a vortex lattice.
16 pages, 12 figures and 3 tables
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- Phase structure of neutron superfluids in strong magnetic fields in neutron stars
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- Non-Abelian Alice strings in two-flavor dense QCD
- Microscopic description of axisymmetric vortices in superfluids
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- Vortex lattice in rotating neutron spin-triplet superfluid
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- Spin-polarized phases of superfluids in neutron stars
- Core structures of vortices in Ginzburg-Landau theory for neutron superfluids
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- Effects of strong magnetic fields on neutron superfluidity with spin-orbit interactions
- Proximity effects of vortices in neutron superfluids in neutron stars: Vortex core transitions and covalent bonding of vortex molecules
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- Two-dimensional Schrödinger symmetry and three-dimensional breathers and Kelvin-ripple complexes as quasi-massive-Nambu-Goldstone modes
- Symmetry classification of uniform states in spin-2 Bose-Einstein condensates and neutron superfluids
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- Emergent chirality and superfluidity of parity-doubled baryons in neutron stars