1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3172
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBhattacharyya, A-
dc.contributor.authorAlam, J-
dc.contributor.authorSarkar, S-
dc.contributor.authorRoy, P-
dc.contributor.authorSinha, B-
dc.contributor.authorRaha, S-
dc.contributor.authorBhattacharjee, P-
dc.date.accessioned2008-08-18T10:41:59Z-
dc.date.available2008-08-18T10:41:59Z-
dc.date.issued1999-12-
dc.identifier.citationNuclear Physics A, Vol. A661, pp. 629c - 632cen
dc.identifier.issn0375-9474-
dc.identifier.urihttp://hdl.handle.net/2248/3172-
dc.description.abstractThe authors calculate the size distribution of quark nuggets, which could be formed due to first order QCD phase transition in the early universe. They find that there are a large number of stable quark nuggets which could be a viable candidate for cosmological dark matter.en
dc.format.extent81569 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherElsevieren
dc.relation.urihttp://arxiv.org/abs/hep-ph/9907262en
dc.subjectDark Matteren
dc.subjectCompositionen
dc.titleCosmological QCD phase transition and dark matteren
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
bhattacharyya.pdf79.66 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.