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Wash-In Leptogenesis
We present a leptogenesis mechanism based on the standard type-I seesaw model that successfully operates at right-handed-neutrino masses as low as a few hundred TeV. This mechanism, which we dub wash-in leptogenesis, does not require any CP violation in the neutrino sector and can be implemented eve...
Autores principales: | , , , , |
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Lenguaje: | eng |
Publicado: |
2020
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevLett.126.201802 http://cds.cern.ch/record/2745099 |
_version_ | 1780968673427587072 |
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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 | We present a leptogenesis mechanism based on the standard type-I seesaw model that successfully operates at right-handed-neutrino masses as low as a few hundred TeV. This mechanism, which we dub wash-in leptogenesis, does not require any CP violation in the neutrino sector and can be implemented even in the regime of strong wash-out. The key idea behind wash-in leptogenesis is to generalize standard freeze-out leptogenesis to a nonminimal cosmological background in which the chemical potentials of all particles not in chemical equilibrium at the temperature of leptogenesis are allowed to take arbitrary values. This sets the stage for building a plethora of new baryogenesis models where chemical potentials generated at high temperatures are reprocessed to generate a nonvanishing B-L asymmetry at low temperatures. As concrete examples, we discuss wash-in leptogenesis after axion inflation and in the context of |
id | cern-2745099 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2020 |
record_format | invenio |
spelling | cern-27450992022-08-10T10:06:09Zdoi:10.1103/PhysRevLett.126.201802http://cds.cern.ch/record/2745099engDomcke, ValerieKamada, KoheiMukaida, KyoheiSchmitz, KaiYamada, MasakiWash-In Leptogenesishep-thParticle Physics - Theoryastro-ph.COAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyWe present a leptogenesis mechanism based on the standard type-I seesaw model that successfully operates at right-handed-neutrino masses as low as a few hundred TeV. This mechanism, which we dub wash-in leptogenesis, does not require any CP violation in the neutrino sector and can be implemented even in the regime of strong wash-out. The key idea behind wash-in leptogenesis is to generalize standard freeze-out leptogenesis to a nonminimal cosmological background in which the chemical potentials of all particles not in chemical equilibrium at the temperature of leptogenesis are allowed to take arbitrary values. This sets the stage for building a plethora of new baryogenesis models where chemical potentials generated at high temperatures are reprocessed to generate a nonvanishing B-L asymmetry at low temperatures. As concrete examples, we discuss wash-in leptogenesis after axion inflation and in the context ofWe present a leptogenesis mechanism based on the standard type-I seesaw model that successfully operates at right-handed-neutrino masses as low as a few 100 TeV. This mechanism, which we dub "wash-in leptogenesis", does not require any CP violation in the neutrino sector and can be implemented even in the regime of strong wash-out. The key idea behind wash-in leptogenesis is to generalize standard freeze-out leptogenesis to a nonminimal cosmological background in which the chemical potentials of all particles not in chemical equilibrium at the temperature of leptogenesis are allowed to take arbitrary values. This sets the stage for building a plethora of new baryogenesis models where chemical potentials generated at high temperatures are reprocessed to generate a nonvanishing B-L asymmetry at low temperatures. As concrete examples, we discuss wash-in leptogenesis after axion inflation and in the context of grand unification.arXiv:2011.09347CERN-TH-2020-196RESCEU-22/20DESY-20-202TU-1112oai:cds.cern.ch:27450992020-11-18 |
spellingShingle | hep-th Particle Physics - Theory astro-ph.CO Astrophysics and Astronomy hep-ph Particle Physics - Phenomenology Domcke, Valerie Kamada, Kohei Mukaida, Kyohei Schmitz, Kai Yamada, Masaki Wash-In Leptogenesis |
title | Wash-In Leptogenesis |
title_full | Wash-In Leptogenesis |
title_fullStr | Wash-In Leptogenesis |
title_full_unstemmed | Wash-In Leptogenesis |
title_short | Wash-In Leptogenesis |
title_sort | wash-in leptogenesis |
topic | hep-th Particle Physics - Theory astro-ph.CO Astrophysics and Astronomy hep-ph Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1103/PhysRevLett.126.201802 http://cds.cern.ch/record/2745099 |
work_keys_str_mv | AT domckevalerie washinleptogenesis AT kamadakohei washinleptogenesis AT mukaidakyohei washinleptogenesis AT schmitzkai washinleptogenesis AT yamadamasaki washinleptogenesis |