The String Landscape, Black Holes and Gravity as the Weakest Force
Nima Arkani-Hamed, Lubos Motl, Alberto Nicolis, Cumrun Vafa

TL;DR
This paper proposes a conjecture that gravity must be weaker than gauge forces in quantum gravity, implying a new ultraviolet scale and the existence of light charged particles, supported by string theory examples and relevant for understanding the limits of effective field theories.
Contribution
It introduces a conjecture relating gravity and gauge forces, predicting a new UV scale and light charged particles, with evidence from string theory.
Findings
Existence of an upper bound on gravity's strength relative to gauge forces.
Presence of a new ultraviolet cutoff scale Lambda=g M_{Pl}.
Support from string theory examples and implications for inflation models.
Abstract
We conjecture a general upper bound on the strength of gravity relative to gauge forces in quantum gravity. This implies, in particular, that in a four-dimensional theory with gravity and a U(1) gauge field with gauge coupling g, there is a new ultraviolet scale Lambda=g M_{Pl}, invisible to the low-energy effective field theorist, which sets a cutoff on the validity of the effective theory. Moreover, there is some light charged particle with mass smaller than or equal to Lambda. The bound is motivated by arguments involving holography and absence of remnants, the (in) stability of black holes as well as the non-existence of global symmetries in string theory. A sharp form of the conjecture is that there are always light "elementary" electric and magnetic objects with a mass/charge ratio smaller than the corresponding ratio for macroscopic extremal black holes, allowing extremal black…
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