Abstract
We show that the strong CP problem is solved in a large class of compactifications of string theory. The Peccei-Quinn mechanism solves the strong CP problem if the CP-breaking effects of the ultraviolet completion of gravity and of QCD are small compared to the CP-preserving axion potential generated by low-energy QCD instantons. We characterize both classes of effects. To understand quantum gravitational effects, we consider an ensemble of flux compactifications of type IIB string theory on orientifolds of Calabi-Yau hypersurfaces in the geometric regime, taking a simple model of QCD on D7-branes. We show that the D-brane instanton contribution to the neutron electric dipole moment falls exponentially in N4, with N the number of axions. In particular, this contribution is negligible in all models in our ensemble with N > 17. We interpret this result as a consequence of large N effects in the geometry that create hierarchies in instanton actions and also suppress the ultraviolet cutoff. We also compute the CP breaking due to high-energy instantons in QCD. In the absence of vectorlike pairs, we find contributions to the neutron electric dipole moment that are not excluded, but that could be accessible to future experiments if the scale of supersymmetry breaking is sufficiently low. The existence of vectorlike pairs can lead to a larger dipole moment. Finally, we show that a significant fraction of models are allowed by standard cosmological and astrophysical constraints.
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Acknowledgments
We thank Csaba Csáki, Jim Halverson, Doddy Marsh, Matt Reece, Max Ruhrdorfer, and Edward Witten for discussions. We are grateful to Richard Nally for comments on a draft of this work. The research of M.D. was supported in part by the National Science Foundation under Cooperative Agreement PHY-2019786 (The NSF AI Institute for Artificial Intelligence and Fundamental Interactions). The research of M.D., N.G., and L.M. was supported in part by NSF grant PHY-1719877, that of C.L. was partially supported by DOE Grant DE-SC0013607, and that of L.M. and J.M. was supported in part by the Simons Foundation Origins of the Universe Initiative.
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Demirtas, M., Gendler, N., Long, C. et al. PQ axiverse. J. High Energ. Phys. 2023, 92 (2023). https://doi.org/10.1007/JHEP06(2023)092
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DOI: https://doi.org/10.1007/JHEP06(2023)092