| dc.contributor.author | Bhattacharyya, Abhijit | |
| dc.contributor.author | Alam, Jan-e | |
| dc.contributor.author | Sarkar, Sourav | |
| dc.contributor.author | Roy, Pradip | |
| dc.contributor.author | Sinha, Bikash | |
| dc.contributor.author | Raha, Sibaji | |
| dc.contributor.author | Bhattacharjee, Pijushpani | |
| dc.date.accessioned | 2012-10-17T08:31:30Z | |
| dc.date.available | 2012-10-17T08:31:30Z | |
| dc.date.issued | 2000-03-16 | |
| dc.identifier | FOR ACCESS PROBLEM CONTACT LIBRARIAN, BOSE INSTITUTE | en_US |
| dc.identifier.citation | Bhattacharyya A, Alam J, Sarkar S, Roy P, Sinha B, Raha S and Bhattacharjee P. (2000) Relics of the cosmological QCD phase transition, Physical Review D61, 083509 | en_US |
| dc.identifier.uri | http://link.aps.org/doi/10.1103/PhysRevD.61.083509 | |
| dc.description | DOI: 10.1103/PhysRevD.61.083509 | en_US |
| dc.description.abstract | The 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_US |
| dc.language.iso | en | en_US |
| dc.publisher | American Physical Society | en_US |
| dc.subject | Relics | en_US |
| dc.subject | cosmological QCD phase transition | en_US |
| dc.subject | cosmological QCD | en_US |
| dc.subject | QCD phase transition | en_US |
| dc.title | Relics of the cosmological QCD phase transition | en_US |
| dc.title.alternative | Physical Review D | en_US |
| dc.type | Article | en_US |
