Pulsar Spin-Down Induced Phenomena: Heating; Magnetic Field Evolution; Glitches; Pulse-Period Modulations

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dc.creatorRuderman, M.
dc.date2001-09-20
dc.date.accessioned2026-07-07T02:00:08Z
dc.date.available2026-07-07T02:00:08Z
dc.descriptionModeling the dynamics of the quantum fluids within a spinning-down neutron star gives a description consistent with observed pulsar magnetic field evolution and spin-period "glitches." The long-standing problem of large predicted excesses in spin-down sustained pulsar heating from such models now see ms resolvable. However, the origin of some pulsar spin-period and pulse-shape modulations which have been interpreted as manifestations of very long period (~year) stellar precession is a crucial challenge to canonical neutron star models.
dc.description10 pages, 4 figures, Invited talk at van Paradijs memorial conference
dc.identifierhttps://arxiv.org/abs/astro-ph/0109353
dc.identifierhttp://arxiv.org/abs/astro-ph/0109353
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3360
dc.subjectAstrophysics
dc.titlePulsar Spin-Down Induced Phenomena: Heating; Magnetic Field Evolution; Glitches; Pulse-Period Modulations
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