UV and IR Effects in Axion Quality Control
C.P. Burgess, Gongjun Choi, F. Quevedo

TL;DR
This paper re-examines the axion quality problem using antisymmetric tensor fields from string theory, showing that the problem is generally avoidable due to UV suppression and multiple field mechanisms.
Contribution
It introduces a duality-based analysis of axion quality, compares different axion types, and identifies conditions under which the quality problem can be evaded.
Findings
UV contributions suppress scalar potential UV sensitivity
Most string vacua fields do not satisfy problematic criteria
Multiple fields can resolve potential axion quality issues
Abstract
Motivated by recent discussions and the absence of exact global symmetries in UV completions of gravity we re-examine the axion quality problem (and naturalness issues more generally) using antisymmetric Kalb-Ramond (KR) fields rather than their pseudoscalar duals, as suggested by string and higher dimensional theories. Two types of axions can be identified: a model independent -type axion dual to a two form in 4D and a -type axion coming directly as 4D scalar Kaluza-Klein (KK) components of higher-dimensional tensor fields. For -type axions our conclusions largely agree with earlier workers for the axion quality problem, but we also reconcile why -type axions can couple to matter localized on 3-branes with Planck suppressed strength even when the axion decay constants are of order the KK scale. For -type axions, we review the duality between form fields and…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories · Solar and Space Plasma Dynamics
