• Open Access

Cosmic implications of a low-scale solution to the axion domain wall problem

Andrea Caputo and Mario Reig
Phys. Rev. D 100, 063530 – Published 23 September 2019

Abstract

The post-inflationary breaking of Peccei-Quinn (PQ) symmetry can lead to the cosmic domain wall catastrophe. In this paper we show how to avoid domain walls by implementing the instanton interference effect with a new interaction which itself breaks PQ symmetry and confines at an energy scale smaller than ΛQCD. We give a general description of the mechanism and consider its cosmological implications and constraints within a minimal model. Contrary to other mechanisms, we do not require an inverse phase transition or fine-tuned bias terms. Incidentally, the mechanism leads to the introduction of new self-interacting dark matter candidates and the possibility of producing gravitational waves in the frequency range of SKA. Unless a fine-tuned hidden sector is introduced, the mechanism predicts a QCD axion in the mass range 1–15 meV.

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  • Received 17 June 2019

DOI:https://doi.org/10.1103/PhysRevD.100.063530

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsGravitation, Cosmology & Astrophysics

Authors & Affiliations

Andrea Caputo* and Mario Reig

  • Instituto de Fisica Corpuscular, Universidad de Valencia and CSIC, Edificio Institutos Investigacion, Catedratico Jose Beltran 2, Paterna, 46980 Spain

  • *andrea.caputo@uv.es
  • mario.reig@ific.uv.es

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Issue

Vol. 100, Iss. 6 — 15 September 2019

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