Deconfinement signals from pulsar timing

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dc.creatorGrigorian, H.
dc.creatorPoghosyan, G.
dc.creatorChubarian, E.
dc.creatorBlaschke, D.
dc.date1999-11-17
dc.date.accessioned2026-07-07T02:34:32Z
dc.date.available2026-07-07T02:34:32Z
dc.descriptionThe occurence of a quark matter core in rotating compact stars has been investigated within general relativity as a function of both the rotational frequency and the total baryon number. We demonstrate that the deviation of the braking index from $n=3$ signals not only the occurence but also the size of a quark matter core in a pulsar. We suggest that in systems with mass accretion onto a rapidly rotating compact star a spin-down to spin-up transition might signal a deconfinement transition in its interior.
dc.description2 pages, 2 eps figures embedded, to be published in Proceedings of IAU Coll. 177: "Pulsar Astronomy - 2000 and Beyond", ASP Conf. Series
dc.identifierhttps://arxiv.org/abs/astro-ph/9911341
dc.identifierhttp://arxiv.org/abs/astro-ph/9911341
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15278
dc.subjectAstrophysics
dc.titleDeconfinement signals from pulsar timing
dc.typetext

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