Tunneling Phenomena in Cosmology: Some Fundamental Problems
| dc.creator | Yoshimura, M. | |
| dc.date | 2000-11-15 | |
| dc.date.accessioned | 2026-07-07T03:43:15Z | |
| dc.date.available | 2026-07-07T03:43:15Z | |
| dc.description | The fundamental problem of how tunneling in thermal medium is completed is addressed, and a new time scale of order 1/friction for its termination, which is usually much shorter than the Hubble time, is pointed out. Enhanced non-linear resonance is responsible for this short time scale. This phenomenon occurs when the semiclassical periodic motion in a metastable potential well resonates with one of the environment harmonic oscillators coupled to its motion. | |
| dc.description | 16 pages, LATEX file. To be published in the Proceedings of COSMO2K (World Scientific) | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0011187 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0011187 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/40148 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Tunneling Phenomena in Cosmology: Some Fundamental Problems | |
| dc.type | text |