| dc.contributor.author | Banerjee, Shibaji | |
| dc.contributor.author | Bhattacharyya, Abhijit | |
| dc.contributor.author | Ghosh, Sanjay Kumar | |
| dc.contributor.author | Raha, Sibaji | |
| dc.contributor.author | Sinha, Bikash | |
| dc.contributor.author | Hiroshi, Toki | |
| dc.date.accessioned | 2012-10-18T08:07:32Z | |
| dc.date.available | 2012-10-18T08:07:32Z | |
| dc.date.issued | 2002-06-20 | |
| dc.identifier | FOR ACCESS PROBLEM CONTACT LIBRARIAN, BOSE INSTITUTE | en_US |
| dc.identifier.citation | Banerjee S., Bhattacharyya A. , Ghosh S. K., Raha S. , Sinha B. , Toki H. (2002), The Cosmic Qcd Phase Transition, Quasi-Baryonic Dark Matter And Massive Compact Halo Objects, astro-ph/ 0206349 | en_US |
| dc.identifier.uri | http://arxiv.org/abs/astro-ph/0206349 | en_US |
| dc.description.abstract | We propose that the cold dark matter (CDM) is composed entirely of quark matter, arising from a cosmic quark-hadron transition. We denote this phase as "quasibaryonic", distinct from the usual baryons. We show that compact gravitational lenses, with masses around 0.5 (M_{\odot}), could have evolved out of the quasibaryonic CDM. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | arXiv.org | en_US |
| dc.subject | Cosmic QCD Phase Transition | en_US |
| dc.subject | Quasi-baryonic Dark Matter | en_US |
| dc.subject | Massive Compact Halo Objects | en_US |
| dc.subject | Cosmic QCD Phase Transition | en_US |
| dc.title | The Cosmic QCD Phase Transition, Quasi-baryonic Dark Matter and Massive Compact Halo Objects | en_US |
| dc.title.alternative | astro-ph | en_US |
| dc.type | Article | en_US |
