Role of Tachyonic Field in Accelerating Universe in Presence of Perfect Fluid
| dc.creator | Chakraborty, Writambhara | |
| dc.creator | Debnath, Ujjal | |
| dc.date | 2008-04-30 | |
| dc.date.accessioned | 2026-07-07T11:50:24Z | |
| dc.date.available | 2026-07-07T11:50:24Z | |
| dc.description | Recently tachyonic field has been depicted as dark energy model to represent the present acceleration of the Universe. In this paper we have considered mixture of tachyonic fluid with a perfect fluid. For this purpose we have considered barotropic fluid and Generalized Chaplygin gas(G.C.G.). We have considered a particular form of the scale factor. We have solved the equations of motion to get the exact solutions of the density, tachyonic potential and the tachyonic field. We have introduced a coupling term to show that the interaction decays with time. Also we have shown that the nature of the potentials vary so as the interaction term reduces the potential in both the cases. | |
| dc.description | 9 latex pages, 4 figures, RevTex style | |
| dc.identifier | https://arxiv.org/abs/0804.4801 | |
| dc.identifier | http://arxiv.org/abs/0804.4801 | |
| dc.identifier | Astrophys.SpaceSci.315:73-78,2008 | |
| dc.identifier | doi:10.1007/s10509-008-9795-6 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/203553 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Role of Tachyonic Field in Accelerating Universe in Presence of Perfect Fluid | |
| dc.type | text |