A Principle to Determine the Number (3 + 1) of Large Spacetime Dimensions
| dc.creator | Rama, S. Kalyana | |
| dc.date | 2006-10-06 | |
| dc.date | 2006-10-18 | |
| dc.date.accessioned | 2026-07-07T11:27:53Z | |
| dc.date.available | 2026-07-07T11:27:53Z | |
| dc.description | We assume that our universe originated from highly excited and interacting strings with coupling constant g_s = {\cal O} (1). Fluctuations of spacetime geometry are large in such strings and the physics dictating the emergence of a final spacetime configuration is not known. We propose that, nevertheless, it is determined by an entropic principle that the final spacetime configuration must have maximum entropy for a given amount of energy. This principle implies, under some assumptions, that the spacetime configuration that emerges finally is a (3 + 1) -- dimensional FRW universe filled with w = 1 perfect fluid and with 6 -- dimensional compact space of size l_s; in particular, the number of large spacetime dimensions is d = 3 + 1. Such an universe may evolve subsequently into our universe, perhaps as in Banks -- Fischler scenario. | |
| dc.description | 11 pages. Latex file. Version 2: References added | |
| dc.identifier | https://arxiv.org/abs/hep-th/0610071 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0610071 | |
| dc.identifier | Phys.Lett.B645:365-368,2007 | |
| dc.identifier | doi:10.1016/j.physletb.2006.11.077 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/196274 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Statistical Mechanics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | A Principle to Determine the Number (3 + 1) of Large Spacetime Dimensions | |
| dc.type | text |