Holographic Vacuum Energy
| dc.creator | Thomas, Scott | |
| dc.date | 2000-10-18 | |
| dc.date | 2002-04-10 | |
| dc.date.accessioned | 2026-07-07T04:10:44Z | |
| dc.date.available | 2026-07-07T04:10:44Z | |
| dc.description | Gravitational holography is argued to render the cosmological constant stable against divergent quantum corrections. This provides a technically natural solution to the cosmological constant problem. Evidence for quantum stability of the cosmological constant is illustrated in a number of examples including, bulk descriptions in terms of delocalized degrees of freedom, boundary screen descriptions on stretched horizons, and non-supersymmetric conformal field theories as dual descriptions of anti-de Sitter space. In an expanding universe, holographic quantum contributions to the stress-energy tensor are argued to be at most of order the energy density of the dominant matter component. | |
| dc.description | 11 pages | |
| dc.identifier | https://arxiv.org/abs/hep-th/0010145 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0010145 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/50316 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Holographic Vacuum Energy | |
| dc.type | text |