Magnetic vortices in a rotating P23 neutron superfluid

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

    Research output: Contribution to journalArticle

    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 languageEnglish (US)
    Pages (from-to)967-975
    Number of pages9
    JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
    Volume25
    Issue number4
    DOIs
    StatePublished - 1982

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    vortices
    neutrons
    relaxation time
    crabs
    pulsars
    neutron stars
    electron scattering
    magnetization
    estimates

    ASJC Scopus subject areas

    • Physics and Astronomy (miscellaneous)

    Cite this

    Magnetic vortices in a rotating P23 neutron superfluid. / Sauls, J. A.; Stein, D. L.; Serene, J. W.

    In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 25, No. 4, 1982, p. 967-975.

    Research output: Contribution to journalArticle

    Sauls, J. A. ; Stein, D. L. ; Serene, J. W. / Magnetic vortices in a rotating P23 neutron superfluid. In: Physical Review D - Particles, Fields, Gravitation and Cosmology. 1982 ; Vol. 25, No. 4. pp. 967-975.
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