Quantization of Gravity Based on a Condensed Matter Model
| dc.creator | Schmelzer, Ilja | |
| dc.date | 1998-07-09 | |
| dc.date | 1998-10-05 | |
| dc.date.accessioned | 2026-07-07T03:32:31Z | |
| dc.date.available | 2026-07-07T03:32:31Z | |
| dc.description | One way the ultraviolet problem may be solved is explicit physical regularization. In this scenario, QFT is only the long distance limit of some unknown non-Poincare-invariant microscopic theory. One can ask how complex and contrived such microscopic theories should be. We show that condensed matter in standard Newtonian framework is sufficient to obtain gravity. We derive a metrical theory of gravity with two additional to GR cosmological constants. The observable difference is similar to homogeneously distributed dark matter with p = -1/3 epsilon. resp. p = epsilon. The gravitational collapse stops before horizon formation and evaporates by Hawking radiation. The cutoff is not the Planck length, but expanding together with the universe. Thus, in some cosmological future microscopic effects become observable. | |
| dc.description | 7 pages Latex, no figures. Sign errors corrected | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9807018 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9807018 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/36262 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Quantization of Gravity Based on a Condensed Matter Model | |
| dc.type | text |