The nano-hertz and milli-hertz stochastic gravitational waves in the minimal clockwork axion model
Xiangwei Yin, Cheng-Wei Chiang, Bo-Qiang Lu, Tianjun Li

TL;DR
This paper proposes a minimal clockwork axion model with multiple domain walls, predicting stochastic gravitational wave signals detectable by current and future experiments, and explores its cosmological and astrophysical constraints.
Contribution
It introduces a novel minimal clockwork axion model with two domain walls, linking gravitational wave signals to specific cosmological phenomena and experimental prospects.
Findings
Nano-hertz GWs from domain wall annihilation detectable by Pulsar Timing Arrays.
Milli-hertz GWs from higher-dimensional operator bias detectable by LISA, Taiji, TianQin.
Model consistent with dark matter, BBN, CMB, and primordial black hole constraints.
Abstract
The clockwork framework can realize TeV-scale symmetry breaking while generating a large axion decay constant \(f_a\). We propose a minimal clockwork axion model with three scalar fields, in which two domain walls (DWs) have non-zero tension. The DW associated with one of the fields is formed following the Peccei-Quinn (PQ) symmetry breaking and subsequently collapses due to the potential bias induced by the QCD instanton. The nano-hertz stochastic gravitational waves (GWs) generated from this DW annihilation can be probed by Pulsar Timing Arrays experiments. In addition, the DW related to the other field is annihilated by a bias potential originating from higher-dimensional operators, producing a significant GW signal with a peak frequency around \(9.41\times10^{-5}\) Hz, which can be detected by the LISA, Taiji, and TianQin experiments. Constraints on the model from…
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Taxonomy
TopicsCosmology and Gravitation Theories · Statistical Mechanics and Entropy · Advanced Thermodynamics and Statistical Mechanics
