Implications for the Cosmological Landscape: Can Thermal Inputs from a Prior Universe Account for Relic Graviton Production?
| dc.creator | Beckwith, A. W. | |
| dc.date | 2008-03-02 | |
| dc.date.accessioned | 2026-07-07T10:16:11Z | |
| dc.date.available | 2026-07-07T10:16:11Z | |
| dc.description | We present a way to accomodate relic graviton production via worm hole transitions of prior universe thermal / energy density values to our present universe. This is done in the context of providing a mechanism for thermally driven relic gravitons, and also to explain how Park's 2003 observation as to how a thermally scaled vacuum energy value plays a role in forming the early universe emergent field dynamics | |
| dc.description | 12 pages, 0 figures, 3 tables, published in the STAIF 2008 conference AIP volume edited by Mohammed El Genik of the University of New Mexico | |
| dc.identifier | https://arxiv.org/abs/0803.0101 | |
| dc.identifier | http://arxiv.org/abs/0803.0101 | |
| dc.identifier | AIPConf.Proc.969:1091-1102,2008 | |
| dc.identifier | doi:10.1063/1.2844947 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/173416 | |
| dc.subject | General Physics | |
| dc.title | Implications for the Cosmological Landscape: Can Thermal Inputs from a Prior Universe Account for Relic Graviton Production? | |
| dc.type | text |