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Neutrino Masses from Outer Space
Neutrinos can gain mass from coupling to an ultralight field in slow roll. When such a field is displaced from its minimum, its vev acts just like the Higgs vev in spontaneous symmetry breaking. Although these masses may eventually vanish, they do it over a very long time. The theory is technically...
Autores principales: | , , |
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Lenguaje: | eng |
Publicado: |
2018
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/j.physletb.2019.134846 http://cds.cern.ch/record/2311940 |
_version_ | 1780957933430898688 |
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author | D'Amico, Guido Hamill, Teresa Kaloper, Nemanja |
author_facet | D'Amico, Guido Hamill, Teresa Kaloper, Nemanja |
author_sort | D'Amico, Guido |
collection | CERN |
description | Neutrinos can gain mass from coupling to an ultralight field in slow roll. When such a field is displaced from its minimum, its vev acts just like the Higgs vev in spontaneous symmetry breaking. Although these masses may eventually vanish, they do it over a very long time. The theory is technically natural, with the ultralight field-dependent part being the right-handed Majorana mass. The mass variation induced by the field correlates with the cosmological evolution. The change of the mass term changes the mixing matrix, and therefore suppresses the fraction of sterile neutrinos at earlier times and increases it at later times. Since the issue of quantum gravity corrections to field theories with large field variations remains open, this framework may give an observational handle on the Weak Gravity Conjecture. |
id | cern-2311940 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2018 |
record_format | invenio |
spelling | cern-23119402023-03-14T17:26:03Zdoi:10.1016/j.physletb.2019.134846http://cds.cern.ch/record/2311940engD'Amico, GuidoHamill, TeresaKaloper, NemanjaNeutrino Masses from Outer Spacehep-thParticle Physics - Theorygr-qcGeneral Relativity and Cosmologyastro-ph.COAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyNeutrinos can gain mass from coupling to an ultralight field in slow roll. When such a field is displaced from its minimum, its vev acts just like the Higgs vev in spontaneous symmetry breaking. Although these masses may eventually vanish, they do it over a very long time. The theory is technically natural, with the ultralight field-dependent part being the right-handed Majorana mass. The mass variation induced by the field correlates with the cosmological evolution. The change of the mass term changes the mixing matrix, and therefore suppresses the fraction of sterile neutrinos at earlier times and increases it at later times. Since the issue of quantum gravity corrections to field theories with large field variations remains open, this framework may give an observational handle on the Weak Gravity Conjecture.arXiv:1804.01542CERN-TH-2018-067oai:cds.cern.ch:23119402018-04-04 |
spellingShingle | hep-th Particle Physics - Theory gr-qc General Relativity and Cosmology astro-ph.CO Astrophysics and Astronomy hep-ph Particle Physics - Phenomenology D'Amico, Guido Hamill, Teresa Kaloper, Nemanja Neutrino Masses from Outer Space |
title | Neutrino Masses from Outer Space |
title_full | Neutrino Masses from Outer Space |
title_fullStr | Neutrino Masses from Outer Space |
title_full_unstemmed | Neutrino Masses from Outer Space |
title_short | Neutrino Masses from Outer Space |
title_sort | neutrino masses from outer space |
topic | hep-th Particle Physics - Theory gr-qc General Relativity and Cosmology astro-ph.CO Astrophysics and Astronomy hep-ph Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1016/j.physletb.2019.134846 http://cds.cern.ch/record/2311940 |
work_keys_str_mv | AT damicoguido neutrinomassesfromouterspace AT hamillteresa neutrinomassesfromouterspace AT kalopernemanja neutrinomassesfromouterspace |