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Lower Limit to the Scale of an Effective Theory of Gravitation

R. R. Caldwell, Daniel Grin

astro-pharXiv:astro-ph/0606133

Abstract

We consider a linearized, effective quantum theory of gravitation in which gravity weakens at energies higher than ~10-3 eV in order to accommodate the apparent smallness of the cosmological constant. Such a theory predicts departures from the static Newtonian inverse-square force law on distances below ~0.05 mm. However, we show that such a modification also leads to changes in the long-range behavior of gravity and is inconsistent with observed gravitational lenses.

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