Observables and cohomology classes for classical gravitational field
| dc.creator | Iftime, M. | |
| dc.date | 2008-09-22 | |
| dc.date.accessioned | 2026-07-07T10:04:20Z | |
| dc.date.available | 2026-07-07T10:04:20Z | |
| dc.description | Some of the most outstanding questions in the field of gravitation and geometry remain unsolved as a result of our limited understanding of the global structure of the spacetime geometry and the role played by global spacetime diffeomorphism group in quantum gravity. Some insight into these important questions may be gained by looking at certain aspects of general covariance and observables in classical gravitational theory. In this paper I shall define as set of classical geometric observables of the gravitational field by which I mean Diff(M)-gauge invariant cohomology classes defined on a Lorentzian structure. They represent global characteristics of the physical gravitational phenomena, are linked to the topology of the spacetime, and can be used in constructing new Lagrangians. The problem of finding a complete set of data out of observables is related perhaps to the fact that at present moment, manifolds in dimension 4 and above cannot be effectively classified. One could interpret this result as a pointer to the possibility that there might be spacetimes with different topologies (i.e., different global characteristics) which have indistinguishable local spacetime geometry. | |
| dc.description | 16 pages. submited | |
| dc.identifier | https://arxiv.org/abs/0809.3596 | |
| dc.identifier | http://arxiv.org/abs/0809.3596 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/169635 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Observables and cohomology classes for classical gravitational field | |
| dc.type | text |