QCD axion window and low-scale inflation

By F. Takahashi, W. Yin, A. Guth. Physical Review D, 2018

140 citations recorded by the source corpus.

We show that the upper bound of the classical QCD axion window can be significantly relaxed for low-scale inflation. If the Gibbons-Hawking temperature during inflation is lower than the QCD scale, the initial QCD axion misalignment angle follows the Bunch-Davies distribution. The distribution is peaked at the strong $CP$ conserving minimum if there is no other light degree of freedom contributing to the strong $CP$ phase. As a result, the axion overproduction problem is significantly relaxed even for an axion decay constant larger than $1{0}^{12}\text{ }\text{ }\mathrm{GeV}$. We also provide concrete hilltop inflation models where the Hubble parameter during inflation is comparable to or much smaller than the QCD scale, with successful reheating taking place via perturbative decays or dissipation processes.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/62fa4183c3da7379dd4babecb04ce323101293fb

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In Astronomy and Astrophysics

  1. A. Ringwald
  2. Igor G. Irastorza
  3. M. Cicoli
  4. G. Ghisellini
  5. F. Tavecchio
  6. Marek Lewicki
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In Nuclear and High Energy Physics

  1. A. Ringwald
  2. M. Cicoli
  3. Igor G. Irastorza
  4. G. Ghisellini
  5. F. Tavecchio
  6. Maurizio Giannotti
  7. J. Redondo
  8. K. Saikawa

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