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Low energy signatures of the TeV scale seesaw mechanism

IBARRA A
•
MOLINARO E
•
Petkov, Serguey
2011
  • journal article

Periodico
PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY
Abstract
We study a type I see-saw scenario where the right-handed (RH) neutrinos, responsible for the light neutrino mass generation, lie at the electroweak scale. Under certain conditions, the strength of the charged (CC) and neutral current (NC) weak interactions of the Standard Model particles with the heavy RH neutrinos can be large enough to allow the production of the latter at the LHC, opening also the possibility of observing other low energy signatures of the new physics in the electroweak precision observables as well as in searches for rare leptonic decays or neutrinoless double beta decay. In this scenario the flavour structure of the indicated CC and NC couplings of the heavy RH neutrinos is essentially determined by the low energy neutrino parameters, leading to fairly strong correlations among the new phenomena. In particular, we show that the present bound on the $\mu\rightarrow e +\gamma$ decay rate makes very difficult the observation of the heavy RH neutrinos at the LHC or the observation of deviations from the Standard Model predictions in the electroweak precision data. We also show that all present experimental constraints on this scenario still allow i) for an enhancement of the rate of neutrinoless double beta decay, which thus can be in the range of sensitivity of the GERDA experiment even when the light Majorana neutrinos possess a normal hierarchical mass spectrum, and ii) for the predicted $\mu\to e+ \gamma$ decay rate to be within the sensitivity range of the MEG experiment.
DOI
10.1103/PhysRevD.84.013005
WOS
WOS:000292514600002
Archivio
http://hdl.handle.net/20.500.11767/16509
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-79961012420
Diritti
closed access
Soggetti
  • TeV scale type I see-...

  • CP violation

  • Dirac neutrinos

  • Gauge theories

  • Settore FIS/02 - Fisi...

Scopus© citazioni
115
Data di acquisizione
Jun 7, 2022
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Web of Science© citazioni
117
Data di acquisizione
Mar 28, 2024
Visualizzazioni
2
Data di acquisizione
Apr 19, 2024
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