Lower Limit to the Scale of an Effective Quantum Theory of Gravitation
Robert R. Caldwell, Daniel Grin
Abstract
Open-access reader
Robert R. Caldwell, Daniel Grin
Abstract
Open-access reader
An effective quantum theory of gravitation in which gravity weakens at energies higher than approximately 10(-3) eV is one way to accommodate the apparent smallness of the cosmological constant. Such a theory predicts departures from the Newtonian inverse-square force law on distances below approximately 0.05 mm. However, it is shown that this modification also leads to changes in the long-range behavior of gravity and is inconsistent with observed gravitational lenses.
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An effective quantum theory of gravitation in which gravity weakens at energies higher than approximately 10(-3) eV is one way to accommodate the apparent smallness of the cosmological constant. Such a theory predicts departures from the Newtonian inverse-square force law on distances below approximately 0.05 mm. However, it is shown that this modification also leads to changes in the long-range behavior of gravity and is inconsistent with observed gravitational lenses.
Key concepts: Inverse-square law, Physics, Gravitation, Quantum gravity, Gravitational constant, Parameterized post-Newtonian formalism, Range (aeronautics), Limit (mathematics)