Magnetic vortices in a rotating P23 neutron superfluid

J. A. Sauls; D. L. Stein; J. W. Serene

doi:10.1103/PhysRevD.25.967

Magnetic vortices in a rotating P23 neutron superfluid

J. A. Sauls, D. L. Stein, J. W. Serene

Research output: Contribution to journal › Article › peer-review

Abstract

P23 vortices in neutron-star matter are structurally different from vortices in a S01 superfluid. The most important difference is that P23 vortices have a spontaneous magnetization in the core region directed along the vortex line. We estimate the velocity relaxation time for electron scattering from these vortices and compare our results with those of Feibelman and the observed relaxation times for the Crab and Vela pulsars.

Original language	English (US)
Pages (from-to)	967-975
Number of pages	9
Journal	Physical Review D
Volume	25
Issue number	4
DOIs	https://doi.org/10.1103/PhysRevD.25.967
State	Published - 1982

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

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10.1103/PhysRevD.25.967

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title = "Magnetic vortices in a rotating P23 neutron superfluid",

abstract = "P23 vortices in neutron-star matter are structurally different from vortices in a S01 superfluid. The most important difference is that P23 vortices have a spontaneous magnetization in the core region directed along the vortex line. We estimate the velocity relaxation time for electron scattering from these vortices and compare our results with those of Feibelman and the observed relaxation times for the Crab and Vela pulsars.",

author = "Sauls, {J. A.} and Stein, {D. L.} and Serene, {J. W.}",

year = "1982",

doi = "10.1103/PhysRevD.25.967",

language = "English (US)",

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journal = "Physical Review D",

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publisher = "American Institute of Physics",

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AU - Sauls, J. A.

AU - Stein, D. L.

AU - Serene, J. W.

PY - 1982

Y1 - 1982

N2 - P23 vortices in neutron-star matter are structurally different from vortices in a S01 superfluid. The most important difference is that P23 vortices have a spontaneous magnetization in the core region directed along the vortex line. We estimate the velocity relaxation time for electron scattering from these vortices and compare our results with those of Feibelman and the observed relaxation times for the Crab and Vela pulsars.

AB - P23 vortices in neutron-star matter are structurally different from vortices in a S01 superfluid. The most important difference is that P23 vortices have a spontaneous magnetization in the core region directed along the vortex line. We estimate the velocity relaxation time for electron scattering from these vortices and compare our results with those of Feibelman and the observed relaxation times for the Crab and Vela pulsars.

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DO - 10.1103/PhysRevD.25.967

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Magnetic vortices in a rotating P23 neutron superfluid

Abstract

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