The Tunneling Hamiltonian Representation of False Vacuum Decay: IV. Application to formation of Dark Matter in nucleating universe
| dc.creator | Beckwith, A. W. | |
| dc.date | 2004-07-28 | |
| dc.date.accessioned | 2026-07-07T04:31:21Z | |
| dc.date.available | 2026-07-07T04:31:21Z | |
| dc.description | The tunneling Hamiltonian has proven to be a useful method in many body physics to treat particle tunneling between different states represented as wavefunctions. Here, we apply a generalization of the way we formed appropriate wave functionals for CDW on how to present nucleation of an inflationary universe. This allows us to make a generalization of the model used for inflation where the infation is trapped in a false vacuum and, after tunning makes a first order phase transition to initiate nucleation of an inflationary universe, in which tunneling between states which are wave functionals between states which wavefunctionals of a scalar quantum field are considered.We explain how we can have particle-anti particle pairs as a model of how nucleation occurs and construct a potential which may permit formation of dark matter using Scherrers k-essence model construction. | |
| dc.description | 27 pages,2 figues | |
| dc.identifier | https://arxiv.org/abs/math-ph/0407070 | |
| dc.identifier | http://arxiv.org/abs/math-ph/0407070 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/57784 | |
| dc.subject | Mathematical Physics | |
| dc.subject | 85A40;81V17 | |
| dc.title | The Tunneling Hamiltonian Representation of False Vacuum Decay: IV. Application to formation of Dark Matter in nucleating universe | |
| dc.type | text |