Bias with a Timer: Axion Domain Wall Decay and Dark Matter
Sally Yuxuan Hao, Shota Nakagawa, Yuichiro Nakai, and Motoo Suzuki

TL;DR
This paper investigates how a light scalar field influences axion domain wall decay and dark matter production, revealing mechanisms that can produce the correct axion dark matter abundance without fine tuning.
Contribution
It introduces a novel scenario where scalar field dynamics affect axion domain wall decay and dark matter generation, expanding understanding of axion cosmology.
Findings
Domain walls can decay via structural instability, not just volume pressure.
Correct axion dark matter abundance achieved with larger decay constants.
Scalar field evolution impacts axion potential and domain wall dynamics.
Abstract
We explore the interplay of the post-inflationary QCD axion and a light scalar field for the axion domain wall decay and dark matter (DM). The scalar field possesses a nonzero vacuum expectation value (VEV) during inflation, so that its interaction with the axion effectively serves as an explicit Peccei-Quinn (PQ) violating term. At a temperature below the PQ phase transition, the effective PQ violating interaction generates the axion potential which generally contains multiple degenerate vacua leading to the formation of the axion string-domain wall networks. The following QCD phase transition provides another contribution to the axion potential making domain walls decay before they dominate the Universe. Later, the scalar field starts to relax to the minimum of its potential with a vanishing VEV, turning off the effective PQ violating interaction so that the axion potential is aligned…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research · Cosmology and Gravitation Theories
