Spinor Theory of Gravity
| dc.creator | Novello, M. | |
| dc.date | 2006-09-08 | |
| dc.date | 2006-10-06 | |
| dc.date.accessioned | 2026-07-07T07:24:00Z | |
| dc.date.available | 2026-07-07T07:24:00Z | |
| dc.description | The proposal of this work is to provide an answer to the following question: is it possible to treat the metric of space-time - that in General Relativity (GR) describes the gravitational interaction - as an effective geometry? In other words, to obtain the dynamics of the metric tensor as a consequence of the dynamics of other fields. In this work we will use a slight modfication of the non-linear equation of motion of a spinor field proposed some years ago by Heisenberg, although in a completely distinct context, to obtain a field theory that provides a framework equivalent to the way GR represents the gravitational interaction. In particular we exhibit a solution of the equations of motion that represents the gravitational field of a compact object and compare it with the corresponding Schwarzschild solution of General Relativity. | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0609033 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0609033 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/116193 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Spinor Theory of Gravity | |
| dc.type | text |