Strangeness in Compact Stars and Signal of Deconfinement

dc.creatorGlendenning, Norman K.
dc.date1997-07-31
dc.date.accessioned2026-07-07T10:51:21Z
dc.date.available2026-07-07T10:51:21Z
dc.descriptionPhase transitions in compact stars are discussed including hyperonization, deconfinement and crystalline phases. Reasons why kaon condensation is unlikely is reviewed. Particular emphasis is placed on the evolution of internal structure with spin-down of pulsars. A signature of a first order phase transition in the timing structure of pulsars which is strong and easy to measure, is identified.
dc.description17 pages, 15 figures, Latex. (Invited Talk at the International Symposium on ``Strangeness In Quark Matter 1997'', Thera (Santorini), Hellas, April 14-18, 1997, To be published in Journal of Physics G (Organizers: A Panagiotou and J. Madsen)
dc.identifierhttps://arxiv.org/abs/astro-ph/9707351
dc.identifierhttp://arxiv.org/abs/astro-ph/9707351
dc.identifierJ.Phys.G23:2013-2027,1997
dc.identifierdoi:10.1088/0954-3899/23/12/026
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/184790
dc.subjectAstrophysics
dc.titleStrangeness in Compact Stars and Signal of Deconfinement
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