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Journal of High Energy Physics

, 2019:120 | Cite as

QCD axion on hilltop by a phase shift of π.

  • Fuminobu Takahashi
  • Wen YinEmail author
Open Access
Regular Article - Theoretical Physics
  • 31 Downloads

Abstract

We show that the initial misalignment angle of the QCD axion (or axion-like particles) can be set very close to π, if the QCD axion has a mixing with another heavy axion which induces the phase shift ≈ π after inflation. In the simplest case, the heavy axion plays the role of the inflaton, and we call such inflation as “πnflation”. The basic idea was first proposed by Daido and the present authors in ref. [1] in 2017 and more recently discussed in ref. [2]. We show that the QCD axion with a decay constant fa ≳ 3 × 109 GeV can explain dark matter by the πnflation mechanism. A large fraction of the parameter region has an overlap with the projected sensitivity of ORGAN, MADMAX, TOORAD and IAXO. We also study implications for the effective neutrino species and isocurvature perturbations. The πnflation can provide an initial condition for the hilltop inflation in the axion landscape, and in a certain set-up, a chain of the hilltop inflation may take place.

Keywords

Cosmology of Theories beyond the SM Beyond Standard Model Discrete Symmetries 

Notes

Open Access

This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited

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Copyright information

© The Author(s) 2019

Authors and Affiliations

  1. 1.Department of PhysicsTohoku UniversitySendaiJapan
  2. 2.Kavli Institute for the Physics and Mathematics of the Universe (WPI)University of TokyoKashiwaJapan
  3. 3.Department of PhysicsKAISTDaejeonSouth Korea

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