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

Nuclear and High Energy Physics

Access to Document

10.1103/PhysRevD.25.967

Cite this

@article{474b6cdbc0df48668fceed64830aedd4,

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)",

volume = "25",

pages = "967--975",

journal = "Physical Review D",

issn = "0556-2821",

publisher = "American Institute of Physics",

number = "4",

}

TY - JOUR

T1 - Magnetic vortices in a rotating P23 neutron superfluid

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.

UR - http://www.scopus.com/inward/record.url?scp=0000105867&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0000105867&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.25.967

DO - 10.1103/PhysRevD.25.967

M3 - Article

AN - SCOPUS:0000105867

SN - 0556-2821

VL - 25

SP - 967

EP - 975

JO - Physical Review D

JF - Physical Review D

IS - 4

ER -

Magnetic vortices in a rotating P23 neutron superfluid

Abstract

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this