Cosmological QCD phase transition and dark matter

dc.contributor.author	Bhattacharyya, A
dc.contributor.author	Alam, J
dc.contributor.author	Sarkar, S
dc.contributor.author	Roy, P
dc.contributor.author	Sinha, B
dc.contributor.author	Raha, S
dc.contributor.author	Bhattacharjee, P
dc.date.accessioned	2008-08-18T10:41:59Z
dc.date.available	2008-08-18T10:41:59Z
dc.date.issued	1999-12
dc.identifier.citation	Nuclear Physics A, Vol. A661, pp. 629c - 632c	en
dc.identifier.issn	0375-9474
dc.identifier.uri	http://hdl.handle.net/2248/3172
dc.description.abstract	The 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.extent	81569 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Elsevier	en
dc.relation.uri	http://arxiv.org/abs/hep-ph/9907262	en
dc.subject	Dark Matter	en
dc.subject	Composition	en
dc.title	Cosmological QCD phase transition and dark matter	en
dc.type	Article	en