Dark-matter induced neutron-antineutron oscillations

Abstract If dark matter carries a baryon number of two, neutron-antineutron oscillations could require its presence to manifest themselves. If it is in addition very light, in the micro-eV range or up to a few orders of magnitude below, these oscillations could even exhibit a Rabi resonance. Though...

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Main Authors: Théo Brugeat, Christopher Smith
Format: Article
Language:English
Published: SpringerOpen 2025-01-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP01(2025)132
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author Théo Brugeat
Christopher Smith
author_facet Théo Brugeat
Christopher Smith
author_sort Théo Brugeat
collection DOAJ
description Abstract If dark matter carries a baryon number of two, neutron-antineutron oscillations could require its presence to manifest themselves. If it is in addition very light, in the micro-eV range or up to a few orders of magnitude below, these oscillations could even exhibit a Rabi resonance. Though the magnetic tuning required to convert a macroscopic number of neutrons into antineutrons is not realistic, sizeable enhancements remain possible. Building on this observation, axionic realizations for this scenario are systematically analyzed. For true QCD axion models, we find that the Goldstone boson nature of the axion imposes the presence of axionless n − n ¯ $$ n-\overline{n} $$ mixing effects, either in vacuum or in decays, which are sufficiently constrained experimentally to leave no room for axion-induced oscillations. Thus, a generic scalar or axion-like dark matter background would have to exist to induce resonant n − n ¯ $$ n-\overline{n} $$ oscillations. Yet, if Nature has taken that path to relate dark matter and baryon number violation, the experimental signature would be striking and certainly worth pursuing.
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spelling doaj-art-be73df9590cd40adb0f98b8a20b82b272025-02-09T12:07:37ZengSpringerOpenJournal of High Energy Physics1029-84792025-01-012025113510.1007/JHEP01(2025)132Dark-matter induced neutron-antineutron oscillationsThéo Brugeat0Christopher Smith1Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble-AlpesLaboratoire de Physique Subatomique et de Cosmologie, Université Grenoble-AlpesAbstract If dark matter carries a baryon number of two, neutron-antineutron oscillations could require its presence to manifest themselves. If it is in addition very light, in the micro-eV range or up to a few orders of magnitude below, these oscillations could even exhibit a Rabi resonance. Though the magnetic tuning required to convert a macroscopic number of neutrons into antineutrons is not realistic, sizeable enhancements remain possible. Building on this observation, axionic realizations for this scenario are systematically analyzed. For true QCD axion models, we find that the Goldstone boson nature of the axion imposes the presence of axionless n − n ¯ $$ n-\overline{n} $$ mixing effects, either in vacuum or in decays, which are sufficiently constrained experimentally to leave no room for axion-induced oscillations. Thus, a generic scalar or axion-like dark matter background would have to exist to induce resonant n − n ¯ $$ n-\overline{n} $$ oscillations. Yet, if Nature has taken that path to relate dark matter and baryon number violation, the experimental signature would be striking and certainly worth pursuing.https://doi.org/10.1007/JHEP01(2025)132Axions and ALPsBaryon/Lepton Number ViolationModels for Dark MatterNew Light Particles
spellingShingle Théo Brugeat
Christopher Smith
Dark-matter induced neutron-antineutron oscillations
Journal of High Energy Physics
Axions and ALPs
Baryon/Lepton Number Violation
Models for Dark Matter
New Light Particles
title Dark-matter induced neutron-antineutron oscillations
title_full Dark-matter induced neutron-antineutron oscillations
title_fullStr Dark-matter induced neutron-antineutron oscillations
title_full_unstemmed Dark-matter induced neutron-antineutron oscillations
title_short Dark-matter induced neutron-antineutron oscillations
title_sort dark matter induced neutron antineutron oscillations
topic Axions and ALPs
Baryon/Lepton Number Violation
Models for Dark Matter
New Light Particles
url https://doi.org/10.1007/JHEP01(2025)132
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