Dynamical Constraints in the Nonsymmetric Gravitational Theory
| dc.creator | Moffat, J. W. | |
| dc.date | 1996-05-08 | |
| dc.date | 2001-08-11 | |
| dc.date.accessioned | 2026-07-07T08:59:34Z | |
| dc.date.available | 2026-07-07T08:59:34Z | |
| dc.description | We impose in the nonsymmetric gravitational theory, by means of Lagrange multiplier fields in the action, a set of covariant constraints on the antisymmetric tensor field. The canonical Hamiltonian constraints in the weak field approximation for the antisymmetric sector yield a Hamiltonian energy bounded from below. An analysis of the Cauchy evolution, in terms of an expansion of the antisymmetric sector about a symmetric Einstein background, shows that arbitrarily small antisymmetric Cauchy data can lead to smooth evolution. | |
| dc.description | 10 pages LaTex. Minor revisions. Results remain the same | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9605016 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9605016 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/147760 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Dynamical Constraints in the Nonsymmetric Gravitational Theory | |
| dc.type | text |