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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3082
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dc.contributor.authorBhattacharyya, A-
dc.contributor.authorAlam, J. E-
dc.contributor.authorSarkar, S-
dc.contributor.authorRoy, P-
dc.contributor.authorSinha, B-
dc.contributor.authorRaha, S-
dc.contributor.authorBhattacharjee, P-
dc.date.accessioned2008-08-12T09:08:42Z-
dc.date.available2008-08-12T09:08:42Z-
dc.date.issued2000-04-
dc.identifier.citationPhysical Review D, Vol. 61, No. 8, pp. 083509en
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/2248/3082-
dc.description.abstractThe abundance and size distribution of quark nuggets ~QN’s!, formed a few microseconds after the big bang due to a first-order QCD phase transition in the early universe, has been estimated. It appears that stable QN’s could be a viable candidate for cosmological dark matter. The evolution of baryon inhomogeneity due to evaporated ~unstable! QN’s is also examined.en
dc.format.extent110929 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.relation.urihttp://link.aps.org/abstract/PRD/v61/e083509en
dc.subjectPhase transitionen
dc.subjectQuark nuggetsen
dc.subjectDark matteren
dc.titleRelics of the cosmological QCD phase transitionen
dc.typeArticleen
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