A Metric Theory of Gravity with Condensed Matter Interpretation
| dc.creator | Schmelzer, I. | |
| dc.date | 2000-01-28 | |
| dc.date | 2000-05-16 | |
| dc.date.accessioned | 2026-07-07T03:24:44Z | |
| dc.date.available | 2026-07-07T03:24:44Z | |
| dc.description | We consider a classical condensed matter theory in a Newtonian framework where conservation laws \partial_t ρ+ \partial_i (ρv^i) = 0 \partial_t (ρv^j) + \partial_i(ρv^i v^j + p^{ij}) = 0 are related with the Lagrange formalism in a natural way. For an ``effective Lorentz metric'' g_{μν} it is equivalent to a metric theory of gravity close to general relativity with Lagrangian L = L_{GR} - (8πG)^{-1}(Υg^{00}-Ξ(g^{11}+g^{22}+g^{33}))\sqrt{-g} We consider the differences between this theory and general relativity (no nontrivial topologies, stable frozen stars instead of black holes, big bounce instead of big bang singularity, a dark matter term), quantum gravity, and the connection with realism and Bohmian mechanics. | |
| dc.description | 16 pages Latex, no figures. Short version of gr-qc/0001101. (The "original" version was a duplicate of gr-qc/0001101 created by a mistake.) | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0001095 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0001095 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/33445 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | A Metric Theory of Gravity with Condensed Matter Interpretation | |
| dc.type | text |