Axion cogenesis without isocurvature perturbations

Co, Raymond T.; Yamada, Masaki

doi:10.1103/physrevd.110.055009

Axion cogenesis without isocurvature perturbations

Journal Article · Wed Sep 04 00:00:00 EDT 2024 · Physical Review. D.

DOI:https://doi.org/10.1103/physrevd.110.055009· OSTI ID:2439646

^[1]; ^[2]

Indiana University, Bloomington, IN (United States); University of Minnesota, Minneapolis, MN (United States)
Tohoku University, Miyagi (Japan)

Axion rotations can simultaneously explain the dark matter abundance and the baryon asymmetry of the Universe by kinetic misalignment and axiogenesis. We consider a scenario in which the Peccei-Quinn symmetry breaking field is as large as the Planck scale during inflation and the axion rotation is initiated by the inflaton-induced potential immediately after the end of inflation. This is a realization of the cogenesis scenario that is free of problems with domain walls and isocurvature perturbations thanks to large explicit Peccei-Quinn symmetry breaking at the Planck scale during inflation. The baryon asymmetry can be more efficiently produced by leptoaxiogenesis, in which case the axion mass is predicted to be larger than O⁡(0.1) meV. We also discuss a UV complete model in supersymmetric theories.

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Research Organization:: University of Minnesota, Minneapolis, MN (United States)

Sponsoring Organization:: JSPS KAKENHI; USDOE

Grant/Contract Number:: SC0011842

OSTI ID:: 2439646

Alternate ID(s):: OSTI ID: 2479324

Journal Information:: Physical Review. D., Journal Name: Physical Review. D. Journal Issue: 5 Vol. 110; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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