Dirac Theory in Space-Time without Torsion
| dc.creator | Hannibal, Ludger | |
| dc.date | 1994-12-08 | |
| dc.date | 1994-12-09 | |
| dc.date.accessioned | 2026-07-07T08:59:27Z | |
| dc.date.available | 2026-07-07T08:59:27Z | |
| dc.description | It is proven that the usual quadratic general-covariant Lagrangian for the Dirac field leads to a symmetric, divergence-free energy-momentum tensor in the standard Riemannian framework of space-time without torsion, provided the tetrad field components are the only quantities related to gravitation that are varied independently. | |
| dc.description | 8 pp, LaTeX | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9412026 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9412026 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/147713 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Dirac Theory in Space-Time without Torsion | |
| dc.type | text |