Chaplygin-Kalb-Ramond Quartessence
| dc.creator | Bilic, Neven | |
| dc.creator | Tupper, Gary B. | |
| dc.creator | Viollier, Raoul D. | |
| dc.date | 2005-04-09 | |
| dc.date | 2005-07-01 | |
| dc.date.accessioned | 2026-07-07T04:18:14Z | |
| dc.date.available | 2026-07-07T04:18:14Z | |
| dc.description | Unified dark matter/energy models (quartessence) based upon the Chaplygin gas D-brane fail owing to the suppression of structure formation by the adiabatic speed of sound. Including string theory effects, in particular the Kalb-Ramond field which becomes massive via the brane, we show how nonadiabatic perturbations allow successful structure formation. | |
| dc.description | 9 pages, substantially expanded, arguments clarified, added references, results unchanged | |
| dc.identifier | https://arxiv.org/abs/hep-th/0504082 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0504082 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/53096 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Chaplygin-Kalb-Ramond Quartessence | |
| dc.type | text |