Can Gravitational Instantons Really Constrain Axion Inflation?
Arthur Hebecker, Patrick Mangat, Stefan Theisen, Lukas T. Witkowski

TL;DR
This paper investigates whether gravitational instantons significantly generate scalar potentials that could challenge axion-based inflation models, concluding that their effects are surprisingly small even in string theory UV completions.
Contribution
It provides a model-independent analysis of gravitational instantons' impact on axion potentials, including detailed calculations and considerations of moduli stabilization and the Weak Gravity Conjecture.
Findings
Gravitational instantons induce a small scalar potential effect.
Explicit calculations show wormholes do not significantly contribute to the potential.
The effect remains small even at the highest string theory scales.
Abstract
Axions play a central role in inflationary model building and other cosmological applications. This is mainly due to their flat potential, which is protected by a global shift symmetry. However, quantum gravity is known to break global symmetries, the crucial effect in the present context being gravitational instantons or Giddings-Strominger wormholes. We attempt to quantify, as model-independently as possible, how large a scalar potential is induced by this general quantum gravity effect. We pay particular attention to the crucial issue which solutions can or cannot be trusted in the presence of a moduli-stabilisation and a Kaluza-Klein scale. An important conclusion is that, due to specific numerical prefactors, the effect is surprisingly small even in UV-completions with the highest possible scale offered by string theory. As we go along, we discuss in detail Euclidean wormholes,…
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