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...

Full description

Bibliographic Details
Main Authors: Kfir Blum, Yosef Nir, Michal Shavit
Format: Article
Language:English
Published: Elsevier 2018-10-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269318306282
id doaj-fb88ca3480b84c1aa57b1f4331f73fa3
record_format Article
spelling 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
_version_ 1725885336882511872