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If heavy neutrinos with mass $m_{ u_{H}}geq$2$ m_e $ are produced in the Sun via the decay ${^8rm{B}} rightarrow {^8rm{Be}} + e^+ + u_H$ in a side branch of pp-chain, they would undergo the observable decay into an electron, a positron and a light neutrino $ u_{H}rightarrow u_{L}+e^++e^-$. In the present work Borexino data are used to set a bound on the existence of such decays. We constrain the mixing of a heavy neutrino with mass 1.5 MeV $leq m_{ u_{H}} le$ 14 MeV to be $|U_{eH}|^2leq (10^{-3}-4times10^{-6})$ respectively. These are tighter limits on the mixing parameters than obtained in previous experiments at nuclear reactors and accelerators.
We present limits on sterile neutrino mixing using 4,438 live-days of atmospheric neutrino data from the Super-Kamiokande experiment. We search for fast oscillations driven by an eV$^2$-scale mass splitting and for oscillations into sterile neutrinos
We study the effects induced by new neutral fermions below their mass threshold, due to their possible mixing with the standard neutrinos. We use as experimental constraints the recent results on lepton universality, together with the measurement of
The OPERA experiment, exposed to the CERN to Gran Sasso $ u_mu$ beam, collected data from 2008 to 2012. Four oscillated $ u_tau$ Charged Current interaction candidates have been detected in appearance mode, which are consistent with $ u_mu to u_tau$
Results are reported from a search for active to sterile neutrino oscillations in the MINOS long-baseline experiment, based on the observation of neutral-current neutrino interactions, from an exposure to the NuMI neutrino beam of $7.07times10^{20}$
A search for resonant absorption of solar axions by $^{169}$Tm nuclei was carried out. A newly developed approach involving low-background cryogenic bolometer based on Tm$_3$Al$_5$O$_{12}$ crystal was used that allowed for significant improvement of