Authors: Carlos Castro
Recently, solutions to the $nonlinear$ Bohm-Poisson (BP) equation were found with relevant cosmological applications. We were able to obtain an exact analytical expression for the observed vacuum energy density, and explain the origins of its $repulsive$ gravitational nature. In this work we considerably improve our prior arguments in support of our findings, and provide further results which include two possible extensions of the Bohm-Poisson equation to the full relativistic regime; explain how Bohm's quantum potential in four-dimensions could be re-interpreted as a gravitational potential in five-dimensions, and which explains why the presence of dark energy/dark matter in our $4D$ spacetime can only be inferred $indirectly$, but not be detected/observed directly. We conclude with some comments about the Dirac-Eddington large numbers coincidences.
Comments: 15 Pages. Submitted to Phys. Letts. B
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