Published October 21, 2015 | Version v1
Journal article

Loop level constraints on Seesaw neutrino mixing

  • 1. Instituto de Física Teórica UAM/CSIC,Calle Nicolás Cabrera 13-15, Cantoblanco E-28049 Madrid (Spain)
  • 2. Departamento de Física Teórica, Universidad Autónoma de Madrid,Cantoblanco E-28049 Madrid (Spain)
  • 3. INFN, sezione di Trieste,34136 Trieste (Italy)
  • 4. Scuola Internazionale Superiore di Studi Avanzati (SISSA), via Bonomea 265, 34136 Trieste (Italy)
  • 5. Laboratoire de Physique Théorique, CNRS - UMR 8627, Université de Paris-Sud,F-91405 Orsay Cedex (France)

Description

We perform a detailed study of the importance of loop corrections when deriving bounds on heavy-active neutrino mixing in the context of general Seesaw mechanisms with extra heavy right-handed neutrinos. We find that, for low-scale Seesaws with an approximate B−L symmetry characterized by electroweak scale Majorana masses and large Yukawas, loop corrections could indeed become relevant in a small part of the parameter space. Previous results in the literature showed that a partial cancellation between these important loop corrections and the tree level contributions could relax some constraints and lead to qualitatively different results upon their inclusion. However, we find that this cancellation can only take place in presence of large violations of the B−L symmetry, that lead to unacceptably large contributions to the light neutrino masses at loop level. Thus, when we restrict our analysis of the key observables to an approximate B−L symmetry so as to recover the correct values for neutrino masses, we always find loop corrections to be negligible in the regions of the parameter space preferred by data.

Availability note (English)

Available from http://dx.doi.org/10.1007/JHEP10(2015)130; Available from http://repo.scoap3.org/record/12368

Additional details

Publishing Information

Journal Title
Journal of High Energy Physics (Online)
Journal Volume
2015
Journal Issue
10
Journal Page Range
p. 130
ISSN
1029-8479

Optional Information

Copyright
Copyright (c) OPEN ACCESS, © The Authors
Notes
PUBLISHER-ID: JHEP10(2015)130; ARXIV:1508.03051; OAI: oai:repo.scoap3.org:12368
Funding organization
SCOAP3, CERN, Geneva (Switzerland)