The double role of Einstein's equations: as equations of motion and as vanishing energy-momentum tensor
| dc.creator | Montesinos, Merced | |
| dc.date | 2003-10-31 | |
| dc.date.accessioned | 2026-07-07T03:28:13Z | |
| dc.date.available | 2026-07-07T03:28:13Z | |
| dc.description | Diffeomorphism covariant theories with dynamical background metric, like gravity coupled to matter fields in the way expressed by Einstein-Hilbert's action or relativistic strings described by Polyakov's action, have `on-shell' vanishing energy-momentum tensor $t_{μν}$ because $t_{μν}$ is, essentially, the Eulerian derivative associated with the dynamical background metric and thus $t_{μν}$ vanishes `on-shell.' Therefore, the equations of motion for the dynamical background metric play a double role: as equations of motion themselves and as a reflection of the fact that $t_{μν}=0$. Alternatively, the vanishing property of $t_{μν}$ can be seen as a reflection of the so-called `problem of time' present in diffeomorphism covariant theories in the sense that $t_{μν}$ are written as linear combinations of first class constraints only. | |
| dc.description | 7 pages, no figures, latex file. Contribution to the meeting in honor of Plebanski. Any comments on this issue are welcome | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0311001 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0311001 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/34742 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Classical Physics | |
| dc.title | The double role of Einstein's equations: as equations of motion and as vanishing energy-momentum tensor | |
| dc.type | text |