A "Running" Gravitational Constant?
| dc.creator | Melissinos, A. C. | |
| dc.date | 2002-07-23 | |
| dc.date | 2002-07-23 | |
| dc.date.accessioned | 2026-07-07T03:47:33Z | |
| dc.date.available | 2026-07-07T03:47:33Z | |
| dc.description | If the gravitational interaction is unified with the electroweak and strong interactions at a mass M=10^15 GeV, the evolution of Newton's constant must differ from its classical (general relativistic) form. We can model such behavior by introducing an ad hoc dependence on ln(s/4m^2) where s is the usual cm energy between two protons. We can then predict the observable effects for relativistic collisions (sqrt(s)~1.4x10^4 GeV) as well as for the case of low velocity motion (beta^2~10^-5) | |
| dc.description | 4 pages | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0207282 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0207282 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/41707 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | A "Running" Gravitational Constant? | |
| dc.type | text |