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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...

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Detalles Bibliográficos
Autores principales: D'Amico, Guido, Hamill, Teresa, Kaloper, Nemanja
Lenguaje:eng
Publicado: 2018
Materias:
Acceso en línea:https://dx.doi.org/10.1016/j.physletb.2019.134846
http://cds.cern.ch/record/2311940
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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.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2018
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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