Neutrinoless double-beta decay with massive scalar emission
Searches for neutrino-less double-beta decay (0ν2β) place an important constraint on models where light fields beyond the Standard Model participate in the neutrino mass mechanism. While 0ν2β experimental collaborations often consider various massless majoron models, including various forms of major...
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doaj-fb88ca3480b84c1aa57b1f4331f73fa32020-11-24T21:50:06ZengElsevierPhysics Letters B0370-26932018-10-01785354361Neutrinoless double-beta decay with massive scalar emissionKfir Blum0Yosef Nir1Michal Shavit2Weizmann Institute, Department of Particle Physics and Astrophysics, Rehovot 7610001, Israel; CERN, Theoretical Physics Department, Switzerland; Corresponding authors.Weizmann Institute, Department of Particle Physics and Astrophysics, Rehovot 7610001, Israel; Corresponding authors.Weizmann Institute, Department of Particle Physics and Astrophysics, Rehovot 7610001, Israel; Corresponding authors.Searches for neutrino-less double-beta decay (0ν2β) place an important constraint on models where light fields beyond the Standard Model participate in the neutrino mass mechanism. While 0ν2β experimental collaborations often consider various massless majoron models, including various forms of majoron couplings and multi-majoron final-state processes, none of these searches considered the scenario where the “majoron” ϕ is not massless, mϕ∼ MeV, of the same order as the Q-value of the 0ν2β reaction. We consider this parameter region and estimate 0ν2βϕ constraints for mϕ of order MeV. The constraints are affected not only by kinematical phase space suppression but also by a change in the signal to background ratio charachterizing the search. As a result, 0ν2βϕ constraints for mϕ>0 diminish significantly below the reaction threshold. This has phenomenological implications, which we illustrate focusing on high-energy neutrino telescopes. The spectral shape of high-energy astrophysical neutrinos could exhibit features due to resonant νν→ϕ→νν scattering. Such features fall within the sensitivity range of IceCube-like experiments, if mϕ is of order MeV, making 0ν2βϕ a key complimentary laboratory constraint on the scenario. Our results motivate a dedicated analysis by 0ν2β collaborations, analogous to the dedicated analyses targeting massless majoron models.http://www.sciencedirect.com/science/article/pii/S0370269318306282 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Kfir Blum Yosef Nir Michal Shavit |
spellingShingle |
Kfir Blum Yosef Nir Michal Shavit Neutrinoless double-beta decay with massive scalar emission Physics Letters B |
author_facet |
Kfir Blum Yosef Nir Michal Shavit |
author_sort |
Kfir Blum |
title |
Neutrinoless double-beta decay with massive scalar emission |
title_short |
Neutrinoless double-beta decay with massive scalar emission |
title_full |
Neutrinoless double-beta decay with massive scalar emission |
title_fullStr |
Neutrinoless double-beta decay with massive scalar emission |
title_full_unstemmed |
Neutrinoless double-beta decay with massive scalar emission |
title_sort |
neutrinoless double-beta decay with massive scalar emission |
publisher |
Elsevier |
series |
Physics Letters B |
issn |
0370-2693 |
publishDate |
2018-10-01 |
description |
Searches for neutrino-less double-beta decay (0ν2β) place an important constraint on models where light fields beyond the Standard Model participate in the neutrino mass mechanism. While 0ν2β experimental collaborations often consider various massless majoron models, including various forms of majoron couplings and multi-majoron final-state processes, none of these searches considered the scenario where the “majoron” ϕ is not massless, mϕ∼ MeV, of the same order as the Q-value of the 0ν2β reaction. We consider this parameter region and estimate 0ν2βϕ constraints for mϕ of order MeV. The constraints are affected not only by kinematical phase space suppression but also by a change in the signal to background ratio charachterizing the search. As a result, 0ν2βϕ constraints for mϕ>0 diminish significantly below the reaction threshold. This has phenomenological implications, which we illustrate focusing on high-energy neutrino telescopes. The spectral shape of high-energy astrophysical neutrinos could exhibit features due to resonant νν→ϕ→νν scattering. Such features fall within the sensitivity range of IceCube-like experiments, if mϕ is of order MeV, making 0ν2βϕ a key complimentary laboratory constraint on the scenario. Our results motivate a dedicated analysis by 0ν2β collaborations, analogous to the dedicated analyses targeting massless majoron models. |
url |
http://www.sciencedirect.com/science/article/pii/S0370269318306282 |
work_keys_str_mv |
AT kfirblum neutrinolessdoublebetadecaywithmassivescalaremission AT yosefnir neutrinolessdoublebetadecaywithmassivescalaremission AT michalshavit neutrinolessdoublebetadecaywithmassivescalaremission |
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