Scales of Gravity

TL;DR

This paper introduces a brane-world model where quantum gravity can be as low as 10^{-3} eV, with a shielding mechanism allowing for weak observable gravity despite a high ultraviolet cutoff.

Contribution

It presents a novel brane-world framework with a shielding effect that maintains weak gravity at large distances even with a low quantum gravity scale.

Findings

Quantum gravity scale can be as low as 10^{-3} eV.

The shielding mechanism prevents strong bulk gravity effects from affecting brane observers.

Experimental signatures include collider signals and deviations in sub-millimeter gravity measurements.

Abstract

We propose a framework in which the quantum gravity scale can be as low as $10^{-3}$ eV. The key assumption is that the Standard Model ultraviolet cutoff is much higher than the quantum gravity scale. This ensures that we observe conventional weak gravity. We construct an explicit brane-world model in which the brane-localized Standard Model is coupled to strong 5D gravity of infinite-volume flat extra space. Due to the high ultraviolet scale, the Standard Model fields generate a large graviton kinetic term on the brane. This kinetic term ``shields'' the Standard Model from the strong bulk gravity. As a result, an observer on the brane sees weak 4D gravity up to astronomically large distances beyond which gravity becomes five-dimensional. Modeling quantum gravity above its scale by the closed string spectrum we show that the shielding phenomenon protects the Standard Model from an apparent phenomenological catastrophe due to the exponentially large number of light string states. The collider experiments, astrophysics, cosmology and gravity measurements {\it independently} point to the same lower bound on the quantum gravity scale, $10^{-3}$ eV. For this value the model has experimental signatures both for colliders and for sub-millimeter gravity measurements. Black holes reveal certain interesting properties in this framework.