Please use this identifier to cite or link to this item: https://hdl.handle.net/10316/4372
DC FieldValueLanguage
dc.contributor.authorMenezes, D. P.-
dc.contributor.authorMelrose, D. B.-
dc.contributor.authorProvidência, C.-
dc.contributor.authorWu, K.-
dc.date.accessioned2008-09-01T11:06:00Z-
dc.date.available2008-09-01T11:06:00Z-
dc.date.issued2007en_US
dc.identifier.citationNuclear Physics A. 790:1-4 (2007) 558c-561cen_US
dc.identifier.urihttps://hdl.handle.net/10316/4372-
dc.description.abstractPhase transitions which can take place in matter at different temperatures and densities are seen in the quantum chromodynamics diagram. The possibility that gamma-ray bursts might result from a phase change in the interior of a pulsar is discussed in the present work. The energy released in the conversion of a metastable star into a stable star is calculated and shown to be of the order of 1050-1053 erg, accounting for both long and short gamma ray bursts.en_US
dc.description.urihttp://www.sciencedirect.com/science/article/B6TVB-4P2S5YJ-41/1/fb6d616877df41309e3835d333c55004en_US
dc.format.mimetypeaplication/PDFen
dc.language.isoengeng
dc.rightsopenAccesseng
dc.titleThe QCD phase diagram and the gamma-ray burstsen_US
dc.typearticleen_US
dc.identifier.doi10.1016/j.nuclphysa.2007.03.094-
uc.controloAutoridadeSim-
item.fulltextCom Texto completo-
item.grantfulltextopen-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairetypearticle-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
crisitem.author.researchunitCFisUC – Center for Physics of the University of Coimbra-
crisitem.author.orcid0000-0001-6464-8023-
Appears in Collections:FCTUC Física - Artigos em Revistas Internacionais
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