Classical gauge theory of gravity
| dc.creator | Sardanashvily, G. | |
| dc.date | 2002-08-19 | |
| dc.date.accessioned | 2026-07-07T03:27:05Z | |
| dc.date.available | 2026-07-07T03:27:05Z | |
| dc.description | The classical theory of gravity is formulated as a gauge theory on a frame bundle with spontaneous symmetry breaking caused by the existence of Dirac fermionic fields. The pseudo-Riemannian metric (tetrad field) is the corresponding Higgs field. We consider two variants of this theory. In the first variant, gravity is represented by the pseudo-Riemannian metric as in general relativity theory; in the second variant, it is represented by the effective metric as in the Logunov relativistic theory of gravity. The configuration space, Dirac operator, and Lagrangians are constructed for both variants. | |
| dc.description | 12 pages | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0208054 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0208054 | |
| dc.identifier | Theor.Math.Phys. 132 (2002) 1163-1171; Teor.Mat.Fiz. 132 (2002) 318-328 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/34299 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Classical gauge theory of gravity | |
| dc.type | text |