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Gravitational Waves and Dark Photon Dark Matter from Axion Rotations

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arxiv 2104.02077 v1 pith:FJGVMOKX submitted 2021-04-05 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords darkaxiongravitationalfieldmatterphotonphotonswaves
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An axion rotating in field space can produce dark photons in the early universe via tachyonic instability. This explosive particle production creates a background of stochastic gravitational waves that may be visible at pulsar timing arrays or other gravitational wave detectors. This scenario provides a novel history for dark photon dark matter. The dark photons may be warm at a level detectable in future 21-cm line surveys. For a consistent cosmology, the radial direction of the complex field containing the axion must be thermalized. We explore a concrete thermalization mechanism in detail and also demonstrate how this setup can be responsible for the generation of the observed baryon asymmetry.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Dark Matter and Baryon Asymmetry from Monopole-Axion Interactions

    hep-ph 2025-11 conditional novelty 8.0 of 10

    A rotating QCD axion dissipates kinetic energy via dark monopole dyon transitions, explaining dark matter and baryon asymmetry with a predicted axion decay constant below 10^9 GeV.

  2. Flipped Rotating Axion Non-minimally Coupled to Gravity: Baryogenesis and Dark Matter

    hep-ph 2025-02 conditional novelty 4.0 of 10

    A rotating axion, kicked into motion by a sign flip in its gravitational effective potential during kination, can co-generate baryon asymmetry and dark matter in a Majoron seesaw model.

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