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Hot axions and the H0 tension

Open access
D'Eramo, Francesco, Ferreira, Ricardo Z., Notari, Alessio, Bernal, José Luis·2018·Journal of Cosmology and Astroparticle Physics

Abstract

Scattering and decay processes of thermal bath particles involving heavy leptons can dump hot axions in the primordial plasma around the QCD phase transition. We compute their relic density, parameterized by an effective number Δ N eff of additional neutrinos. For couplings allowed by current bounds, production via scattering yields Δ N eff ≲ 0.6 and Δ N eff ≲ 0.2 for the cases of muon and tau, respectively. Flavor violating tau decays to a lighter lepton plus an axion give Δ N eff ≲ 0.3. Such values of Δ N eff can alleviate the tension between the direct local measurement of the Hubble constant H 0 and the inferred value from observations of the Cosmic Microwave Background, assuming ΛCDM . We analyze present cosmological data from the Planck collaboration and baryon acoustic oscillations with priors given in terms of the axion-lepton couplings. For axions coupled to muons, the tension can be alleviated below the 3σ level. Future experiments will measure Δ N eff with higher precision, providing an axion discovery channel and probing the role of hot axions in the H 0 tension.

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Metadata

Authors
D'Eramo, F., Ferreira, R. Z., Notari, A., & Bernal, J. L.
Venue
Journal of Cosmology and Astroparticle Physics
Published
2018-11-12
Volume
2018
Issue
11
Pages
014-014
ISSN
  • 1475-7508 (ISSN-L)
  • 1475-7516
OpenAlex
W2888247039
Cited by
174
References
3
FWCI
12.26
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Hot axions and the H0 tension. https://app.cochat.ai/papers/10.1088/1475-7516/2018/11/014
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D'Eramo, F., Ferreira, R. Z., Notari, A., & Bernal, J. L. (2018). Hot axions and the H0 tension. Journal of Cosmology and Astroparticle Physics. https://doi.org/10.1088/1475-7516/2018/11/014

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