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Short-Baseline Electron Neutrino Oscillation Length After Troitsk

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arxiv 1212.3805 v2 pith:CL5EF7WM submitted 2012-12-16 hep-ph astro-ph.COhep-ex

classification hep-phastro-ph.COhep-ex
keywords neutrinoshort-baselinetroitskdisappearancediscusselectronexperimentsimplications
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We discuss the implications for short-baseline electron neutrino disappearance in the 3+1 mixing scheme of the recent Troitsk bounds on the mixing of a neutrino with mass between 2 and 100 eV. Considering the Troitsk data in combination with the results of short-baseline nu_e and antinu_e disappearance experiments, which include the reactor and Gallium anomalies, we derive a 2 sigma allowed range for the effective neutrino squared-mass difference between 0.85 and 43 eV^2. The upper bound implies that it is likely that oscillations in distance and/or energy can be observed in radioactive source experiments. It is also favorable for the ICARUS@CERN experiment, in which it is likely that oscillations are not washed-out in the near detector. We discuss also the implications for neutrinoless double-beta decay.

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    Cosmological limits still allow an eV-scale sterile neutrino if ultralight dark matter gives it a large early-universe mass, with an early mass above about 160 eV.

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