Lepto-axiogenesis with light right-handed neutrinos

Fuente: arXiv
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Auteurs principaux: Barnes, Patrick, Co, Raymond T., Harigaya, Keisuke, Pierce, Aaron
Format: Preprint
Publié: 2024
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author Barnes, Patrick
Co, Raymond T.
Harigaya, Keisuke
Pierce, Aaron
author_facet Barnes, Patrick
Co, Raymond T.
Harigaya, Keisuke
Pierce, Aaron
contents We study lepto-axiogenesis in theories where the right-handed neutrino is light enough that its dynamics affect the determination of the baryon asymmetry. When compared with theories of high-scale lepto-axiogenesis where the Majorana neutrino mass may be treated as an effective dimension-five operator, we find that the predicted saxion mass is lower. Two distinct scenarios emerge. In the first, processes that generate the baryon asymmetry are in equilibrium down to the mass of the right-handed neutrino. In the second, the relevant processes never reach equilibrium; the baryon number freezes in. We comment on implications for supersymmetric spectra and discuss constraints on late decays of supersymmetric relics and from dark radiation. In contrast to high-scale lepto-axiogenesis, which predicts superpartners with masses of 10-100 TeV or more, we find this scenario is consistent with a wider range of superpartner masses, all the way down to current direct search bounds.
format Preprint
id arxiv_https___arxiv_org_abs_2402_10263
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Lepto-axiogenesis with light right-handed neutrinos
Barnes, Patrick
Co, Raymond T.
Harigaya, Keisuke
Pierce, Aaron
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
We study lepto-axiogenesis in theories where the right-handed neutrino is light enough that its dynamics affect the determination of the baryon asymmetry. When compared with theories of high-scale lepto-axiogenesis where the Majorana neutrino mass may be treated as an effective dimension-five operator, we find that the predicted saxion mass is lower. Two distinct scenarios emerge. In the first, processes that generate the baryon asymmetry are in equilibrium down to the mass of the right-handed neutrino. In the second, the relevant processes never reach equilibrium; the baryon number freezes in. We comment on implications for supersymmetric spectra and discuss constraints on late decays of supersymmetric relics and from dark radiation. In contrast to high-scale lepto-axiogenesis, which predicts superpartners with masses of 10-100 TeV or more, we find this scenario is consistent with a wider range of superpartner masses, all the way down to current direct search bounds.
title Lepto-axiogenesis with light right-handed neutrinos
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2402.10263