A Metric Theory of Gravity with Condensed Matter Interpretation
  We consider a classical condensed matter theory in a Newtonian framework where conservation laws   \partial_t \rho + \partial_i (\rho v^i) = 0   \partial_t (\rho v^j) + \partial_i(\rho v^i v^j + p^{ij}) = 0   are related with the Lagrange formalism in a natural way. For an ``effective Lorentz metric'' g_{\mu\nu} it is equivalent to a metric theory of gravity close to general relativity with Lagrangian   L = L_{GR}   - (8\pi G)^{-1}(\Upsilon g^{00}-\Xi (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. 
I. Schmelzer