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@ARTICLE{Merle:172437,
      author       = {Merle, Alexander and Morisi, Stefano and Winter, Walter},
      title        = {{C}ommon origin of reactor and sterile neutrino mixing},
      journal      = {Journal of high energy physics},
      volume       = {2014},
      number       = {7},
      issn         = {1029-8479},
      address      = {Berlin},
      publisher    = {Springer},
      reportid     = {PUBDB-2014-03736, arXiv:1402.6332},
      pages        = {39},
      year         = {2014},
      note         = {OA},
      abstract     = {If the hints for light sterile neutrinos from
                      short-baseline anomalies are to be taken seriously, global
                      fits indicate active-sterile mixings of a magnitude
                      comparable to the known reactor mixing. We therefore study
                      the conditions under which the active-sterile and reactor
                      mixings could have the same origin in an underlying flavour
                      model. As a starting point, we use $\mu-\tau$ symmetry in
                      the active neutrino sector, which (for three neutrinos)
                      yields a zero reactor neutrino angle and a maximal
                      atmospheric one. We demonstrate that adding one sterile
                      neutrino can change this setting, so that the active-sterile
                      mixing and non-zero $\theta_{13}$ can be generated
                      simultaneously. From the phenomenological perspective,
                      electron (anti)neutrino disappearance can be easily
                      accommodated, while muon neutrino disappearance can vanish.
                      It is, however, difficult to reconcile the LSND results with
                      this scenario. From the theory perspective, the setting
                      requires the misalignment of some of the flavon vacuum
                      expectation values, which may be achieved in an $A_4$ or
                      $D_4$ flavour symmetry model using extra dimensions.},
      cin          = {$Z_THAT$},
      ddc          = {530},
      cid          = {$I:(DE-H253)Z_THAT-20210408$},
      pnm          = {52x - Programm Astroteilchenphysik - Topic unbekannt
                      (POF2-52x) / INVISIBLES - INVISIBLES (289442) / THE TRUE
                      PATH BEYOND - Finding the True Path Beyond the Standard
                      Model (297557)},
      pid          = {G:(DE-HGF)POF2-52x / G:(EU-Grant)289442 /
                      G:(EU-Grant)297557},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)29 / PUB:(DE-HGF)16},
      eprint       = {1402.6332},
      howpublished = {arXiv:1402.6332},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1402.6332;\%\%$},
      UT           = {WOS:000339422600001},
      doi          = {10.1007/JHEP07(2014)039},
      url          = {https://bib-pubdb1.desy.de/record/172437},
}