2013
DOI: 10.1007/jhep05(2013)050
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Sterile neutrino oscillations: the global picture

Abstract: Neutrino oscillations involving eV-scale neutrino mass states are investigated in the context of global neutrino oscillation data including short and long-baseline accelerator, reactor, and radioactive source experiments, as well as atmospheric and solar neutrinos. We consider sterile neutrino mass schemes involving one or two mass-squared differences at the eV 2 scale denoted by 3+1, 3+2, and 1+3+1. We discuss the hints for eV-scale neutrinos from ( -) ν e disappearance (reactor and Gallium anomalies) and ( -… Show more

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Cited by 452 publications
(602 citation statements)
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“…Moreover, these contributions are associated to light sterile states: as can be seen from the right panel of figure 3, contributions within the 3σ interval correspond to m 4 10 −2 GeV. The two vertical lines of the right panel JHEP09(2014)074 denote the values of the mostly (lightest) sterile state mass that would allow to address issues strongly motivating these extensions of the SM: (i) m 4 1 eV, the best fit value for a sterile state accounting for the reactor anomaly [100]; (ii) m 4 ∼ 7 keV, as required to explain the 3.5 keV line in the X-ray spectra of galaxy clusters from the decay of a warm dark matter candidate [89,90]. We stress that this is a simple, minimal extension and that the analysis relies on a first order (one-loop) computation of the observable.…”
Section: Results: "3+1" Effective Modelmentioning
confidence: 99%
“…Moreover, these contributions are associated to light sterile states: as can be seen from the right panel of figure 3, contributions within the 3σ interval correspond to m 4 10 −2 GeV. The two vertical lines of the right panel JHEP09(2014)074 denote the values of the mostly (lightest) sterile state mass that would allow to address issues strongly motivating these extensions of the SM: (i) m 4 1 eV, the best fit value for a sterile state accounting for the reactor anomaly [100]; (ii) m 4 ∼ 7 keV, as required to explain the 3.5 keV line in the X-ray spectra of galaxy clusters from the decay of a warm dark matter candidate [89,90]. We stress that this is a simple, minimal extension and that the analysis relies on a first order (one-loop) computation of the observable.…”
Section: Results: "3+1" Effective Modelmentioning
confidence: 99%
“…2 The analyses performed in [19,37] with the existing data from T2K and NOνA have already shown that these two experiments 3 can probe one of the new CP-phases for realistic values of the mixing angles indicated by the global 3+1 fits [42,43]. In addition, in [37] it has been pointed out that the statistical significance of the current indications concerning the standard CP-phase δ and the neutrino mass hierarchy is modified (reduced) in the presence of sterile neutrinos.…”
Section: Jhep02(2016)111mentioning
confidence: 92%
“…The first of the two interference terms is connected to the standard solar-atmospheric interference, while the second one is driven by the atmospheric-sterile interference. The conversion probability depends on the three small mixing angles θ 13 , θ 14 , θ 24 , whose best estimates, derived from the global 3-flavor (for θ 13 ) analyses [44][45][46] and from the 3+1 fits [42,43] where ∆ ≡ ∆m 2 31 L/4E is the atmospheric oscillating factor, which depends on the baseline L and the neutrino energy E. The two LBL experiments under consideration, T2K and NOνA, make use of an off-axis configuration, which leads to a narrow-band sharply-peaked energy spectrum of the emitted neutrinos. In theory, the off-axis angle should be tuned exactly to match (at the peak energy) the condition ∆ ∼ π/2, corresponding to the first oscillation maximum.…”
Section: Analytical Expressions In Vacuum and Mattermentioning
confidence: 99%
“…This would imply that instead of the three-neutrino mixing scheme (in oscillation phenomena), one would have a 3 + 1-neutrino (or 3+more) mixing schemes (see, for instance, [33]). …”
Section: Jhep08(2016)079mentioning
confidence: 99%