Cosmological parameters from the thermodynamic model of gravity
arXiv:1210.4618 · doi:10.1007/s10773-013-1976-6
Abstract
Within our recent thermodynamic model of gravity the dark energy is identified with the energy of collective gravitational interactions of all particles in the universe, which is missing in the standard treatments. For a simple model universe composed of neutral and charged particles of identical mass we estimate the radiation, baryon and dark energy densities and obtain the values which are very close to the current cosmological observations.
v2: The final version to appear in IJTP, minor linguistic improvements
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