A Hagedorn temperature in post-inflationary dynamics?
| dc.creator | Jaikumar, Prashanth | |
| dc.creator | Mazumdar, Anupam | |
| dc.date | 2003-09-15 | |
| dc.date | 2003-09-22 | |
| dc.date.accessioned | 2026-07-07T03:50:38Z | |
| dc.date.available | 2026-07-07T03:50:38Z | |
| dc.description | We consider the possibility of regarding the maximum temperature $\tm$ of a plasma of inflaton decay products as a Hagedorn temperature connected with the transition from an inflaton-dominated epoch to a radiation-dominated universe. Employing a ``bottom-up'' approach to inflaton decay, we show that the limiting temperature $T_{\rm H}\sim m_ϕ$, as obtained from a numerical analysis of the evolution equations, can also be understood theoretically in a Hagedorn picture of the phase transition. | |
| dc.description | 4 pages, 1 figure, one refernce added and typos corrected | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0309175 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0309175 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/42844 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.title | A Hagedorn temperature in post-inflationary dynamics? | |
| dc.type | text |