Spin-up of Solitary Pulsars: Signal of Deconfinement

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dc.creatorGlendenning, Norman K.
dc.date1998-03-06
dc.date.accessioned2026-07-07T02:26:18Z
dc.date.available2026-07-07T02:26:18Z
dc.descriptionA phase transition in the nature of matter in the core of a neutron star, such as quark deconfinement or Bose condensation, can cause the spontaneous spin-up of a solitary millisecond pulsar. The spin-up epoch for our model lasts for $2\times 10^7$ years or 1/50 of the spin-down time.
dc.description7 pages, 4 figures, Latex (To be published in Proceedings of `Neutron Stars and Pulsars' November 1997, Tokyo by Universal Academy Press
dc.identifierhttps://arxiv.org/abs/astro-ph/9803070
dc.identifierhttp://arxiv.org/abs/astro-ph/9803070
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12217
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleSpin-up of Solitary Pulsars: Signal of Deconfinement
dc.typetext

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