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Clockwork axion footprint on nanohertz stochastic gravitational wave background

Bo-Qiang Lu1,*, Cheng-Wei Chiang2,3,†, and Tianjun Li4,5,‡

  • 1School of Science, Huzhou University, Huzhou, Zhejiang 313000, People’s Republic of China
  • 2Department of Physics and Center for Theoretical Physics, National Taiwan University, Taipei 10617, Taiwan
  • 3Physics Division, National Center for Theoretical Sciences, Taipei 10617, Taiwan
  • 4CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, People’s Republic of China
  • 5School of Physical Sciences, University of Chinese Academy of Sciences, No. 19A Yuquan Road, Beijing 100049, People’s Republic of China

  • *bqlu@zjhu.edu.cn
  • †chengwei@phys.ntu.edu.tw
  • ‡tli@itp.ac.cn

Phys. Rev. D 109, L101304 – Published 16 May, 2024

DOI: https://doi.org/10.1103/PhysRevD.109.L101304

Abstract

The recent pulsar timing arrays (PTAs) nano-Hz gravitational wave (GW) background signal can be naturally induced by the annihilation of domain walls (DWs) formed at a symmetry-breaking scale f≃200  TeV in the clockwork axion framework. Based on our first successful and precise prediction, we, for the first time, suggest that the recent PTA observations strongly support the novel mechanism of the QCD instanton-induced DW annihilation in the clockwork axion framework. We also, for the first time, discover a novel correlation between dark matter relic abundance and nano-Hz GW background, which in turn indicates a natural connection between the axion decay constant and the symmetry-breaking scale in the clockwork framework. We find that the GW signal has a peak h2ΩGW≃10−6.6−10−6.1 at about 50 nHz, which is definite and testable for future PTA data at frequencies ≳25  nHz and CMB-S4 experiment. We also propose various phenomena that may appear in PTAs and future GW interferometers.

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