Quantum gravity at very high energies
Abstract
The problem of time and the quantization of three-dimensional gravity in the strong coupling regime is studied following path integral methods. The time is identified with the volume of spacetime. We show that the effective action describes an infinite set of massless relativistic particles moving in a curved three-dimensional target space, i.e., a tensionless 3-brane on a curved background. If the cosmological constant is zero the target space is flat and there is no '' graviton" propagation (i.e., G[gij(2),gij(1)]=0). If the cosmological constant is different from zero, 3D gravity is both classical and quantum mechanically soluble. Indeed, we find the following results: (i) the general exact solutions of the Einstein equations are singular at t=0 showing the existence of a big-bang in this regime and (ii) the propagation amplitude between two geometries ?gij(2),t2|gij(1),t1? vanishes as t?0, suggesting that big-bang is suppressed quantum mechanically. This result is also valid for D>3.
Más información
Título según WOS: | Quantum gravity at very high energies |
Título según SCOPUS: | Quantum gravity at very high energies |
Título de la Revista: | NUCLEAR PHYSICS B |
Volumen: | 600 |
Número: | 2 |
Editorial: | ELSEVIER SCIENCE BV |
Fecha de publicación: | 2001 |
Página de inicio: | 378 |
Página final: | 386 |
Idioma: | English |
URL: | http://linkinghub.elsevier.com/retrieve/pii/S0550321301000840 |
DOI: |
10.1016/S0550-3213(01)00084-0 |
Notas: | ISI, SCOPUS |