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Wash-in leptogenesis after axion inflation

CP violation and the violation of baryon-minus-lepton number B−L do not necessarily have to occur simultaneously in order to accomplish successful leptogenesis. Instead, it suffices if new CP-violating interactions at high energies result in primordial charge asymmetries, which are then reprocessed...

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Autores principales: Domcke, Valerie, Kamada, Kohei, Mukaida, Kyohei, Schmitz, Kai, Yamada, Masaki
Lenguaje:eng
Publicado: 2022
Materias:
Acceso en línea:https://dx.doi.org/10.1007/JHEP01(2023)053
http://cds.cern.ch/record/2836838
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author Domcke, Valerie
Kamada, Kohei
Mukaida, Kyohei
Schmitz, Kai
Yamada, Masaki
author_facet Domcke, Valerie
Kamada, Kohei
Mukaida, Kyohei
Schmitz, Kai
Yamada, Masaki
author_sort Domcke, Valerie
collection CERN
description CP violation and the violation of baryon-minus-lepton number B−L do not necessarily have to occur simultaneously in order to accomplish successful leptogenesis. Instead, it suffices if new CP-violating interactions at high energies result in primordial charge asymmetries, which are then reprocessed into a nonvanishing B−L asymmetry by right-handed neutrinos (RHNs) at lower energies. In this paper, we study this novel mechanism known as wash-in leptogenesis, utilizing axion inflation as the source of high-scale CP violation. We specifically consider axion inflation coupled to the Standard Model hypercharge sector, which results in the dual production of hypermagnetic helicity and fermionic charge asymmetries. Although the survival of these charges is endangered by sphaleron processes, magnetic diffusion, and the chiral plasma instability, we find a large range of viable scenarios. We consistently account for RHN flavor effects and coherence among the Standard Model lepton flavors across a wide range of RHN masses. We find a lower bound of 10$^{5···9}$ GeV on the mass of the lightest RHN involved in wash-in leptogenesis, depending on the onset of turbulence in the chiral plasma and the Hubble scale of inflation. Our model is representative of a broader class of new leptogenesis scenarios and suggests interesting observational signatures with regard to intergalactic magnetic fields, primordial black holes, and gravitational waves.
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spelling cern-28368382023-03-12T05:39:01Zdoi:10.1007/JHEP01(2023)053http://cds.cern.ch/record/2836838engDomcke, ValerieKamada, KoheiMukaida, KyoheiSchmitz, KaiYamada, MasakiWash-in leptogenesis after axion inflationastro-ph.COAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyCP violation and the violation of baryon-minus-lepton number B−L do not necessarily have to occur simultaneously in order to accomplish successful leptogenesis. Instead, it suffices if new CP-violating interactions at high energies result in primordial charge asymmetries, which are then reprocessed into a nonvanishing B−L asymmetry by right-handed neutrinos (RHNs) at lower energies. In this paper, we study this novel mechanism known as wash-in leptogenesis, utilizing axion inflation as the source of high-scale CP violation. We specifically consider axion inflation coupled to the Standard Model hypercharge sector, which results in the dual production of hypermagnetic helicity and fermionic charge asymmetries. Although the survival of these charges is endangered by sphaleron processes, magnetic diffusion, and the chiral plasma instability, we find a large range of viable scenarios. We consistently account for RHN flavor effects and coherence among the Standard Model lepton flavors across a wide range of RHN masses. We find a lower bound of 10$^{5···9}$ GeV on the mass of the lightest RHN involved in wash-in leptogenesis, depending on the onset of turbulence in the chiral plasma and the Hubble scale of inflation. Our model is representative of a broader class of new leptogenesis scenarios and suggests interesting observational signatures with regard to intergalactic magnetic fields, primordial black holes, and gravitational waves.CP violation and the violation of baryon-minus-lepton number B-L do not necessarily have to occur simultaneously in order to accomplish successful leptogenesis. Instead, it suffices if new CP-violating interactions at high energies result in primordial charge asymmetries, which are then reprocessed into a nonvanishing B-L asymmetry by right-handed neutrinos (RHNs) at lower energies. In this paper, we study this novel mechanism known as "wash-in leptogenesis", utilizing axion inflation as the source of high-scale CP violation. We specifically consider axion inflation coupled to the Standard Model hypercharge sector, which results in the dual production of hypermagnetic helicity and fermionic charge asymmetries. Although the survival of these charges is endangered by sphaleron processes, magnetic diffusion, and the chiral plasma instability, we find a large range of viable scenarios. We consistently account for RHN flavor effects and coherence among the Standard Model lepton flavors across a wide range of RHN masses. We find a lower bound of 10^(5...9) GeV on the mass of the lightest RHN involved in wash-in leptogenesis, depending on the onset of turbulence in the chiral plasma and the Hubble scale of inflation. Our model is representative of a broader class of new leptogenesis scenarios and suggests interesting observational signatures with regard to intergalactic magnetic fields, primordial black holes, and gravitational waves.arXiv:2210.06412CERN-TH-2022-162RESCEU-17/22KEK-TH-2455MS-TP-22-37TU-1170oai:cds.cern.ch:28368382022-10-12
spellingShingle astro-ph.CO
Astrophysics and Astronomy
hep-ph
Particle Physics - Phenomenology
Domcke, Valerie
Kamada, Kohei
Mukaida, Kyohei
Schmitz, Kai
Yamada, Masaki
Wash-in leptogenesis after axion inflation
title Wash-in leptogenesis after axion inflation
title_full Wash-in leptogenesis after axion inflation
title_fullStr Wash-in leptogenesis after axion inflation
title_full_unstemmed Wash-in leptogenesis after axion inflation
title_short Wash-in leptogenesis after axion inflation
title_sort wash-in leptogenesis after axion inflation
topic astro-ph.CO
Astrophysics and Astronomy
hep-ph
Particle Physics - Phenomenology
url https://dx.doi.org/10.1007/JHEP01(2023)053
http://cds.cern.ch/record/2836838
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AT mukaidakyohei washinleptogenesisafteraxioninflation
AT schmitzkai washinleptogenesisafteraxioninflation
AT yamadamasaki washinleptogenesisafteraxioninflation