English

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

High Energy Physics - Phenomenology 2019-10-02 v2 Cosmology and Nongalactic Astrophysics

Abstract

The post-inflationary breaking of Peccei-Quinn (PQ) symmetry can lead to the cosmic domain wall catastrophe. In this Letter we show how to avoid domain walls implementing the Instanton Interference Effect (IIE) with a new interaction which itself breaks PQ symmetry and confines at an energy scale smaller than ΛQCD\Lambda_{QCD}. 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 neither 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 meV15 meV1\text{ meV}-15\text{ meV}.

Keywords

Cite

@article{arxiv.1905.13116,
  title  = {Cosmic implications of a low-scale solution to the axion domain wall problem},
  author = {Andrea Caputo and Mario Reig},
  journal= {arXiv preprint arXiv:1905.13116},
  year   = {2019}
}

Comments

12 pages, 4 figures; matches published version