Gauge Unified Theories without the Cosmological Constant Problem
| dc.creator | Guendelman, E. I. | |
| dc.creator | Kaganovich, A. B. | |
| dc.date | 1998-03-17 | |
| dc.date.accessioned | 2026-07-07T04:24:21Z | |
| dc.date.available | 2026-07-07T04:24:21Z | |
| dc.description | We study gauge theories in the context of a gravitational theory without the cosmological constant problem (CCP). The theory is based on the requirement that the measure of integration in the action is not necessarily $\sqrt{-g}$ but it is determined dynamically through additional degrees of freedom. Realization of these ideas in the framework of the first order formalism solves the CCP. Incorporation of a condensate of a four index field strength allows, after a conformal transformation to the Einstein frame, to represent the system of gravity and matter in the standard GR form. Now, however, the effective potential vanishes at a vacuum state due to the exact balance to zero of the gauge fields condensate and the original scalar fields potential. As a result it is possible to combine the solution of the CCP with: a) inflation and transition to a $Λ=0$ phase without fine tuning after a reheating period; b) spontaneously broken gauge unified theories (including fermions). The model opens new possibilities for a solution of the hierarchy problem. | |
| dc.description | LaTeX, 25 pages | |
| dc.identifier | https://arxiv.org/abs/hep-th/9803134 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9803134 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/55380 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Gauge Unified Theories without the Cosmological Constant Problem | |
| dc.type | text |