Experimental bounds on the neutrino lifetime depend on the nature of the neutrinos and the details of the potentially new physics responsible for neutrino decay. In the case where the decays involve active neutrinos in the final state, the neutrino masses also qualitatively impact how these manifest themselves experimentally. In order to further understand the impact of nonzero neutrino masses, we explore how observations of solar neutrinos constrain a very simple toy model. We assume that neutrinos are Dirac fermions and there is a new massless scalar that couples to neutrinos such that a heavy neutrino— with mass —can decay into a lighter neutrino— with mass —and a massless scalar. We find that the constraints on the new physics coupling depend, sometimes significantly, on the ratio of the daughter-to-parent neutrino masses and that, for large-enough values of the new physics coupling, the “dark side” of the solar neutrino parameter space— —provides a reasonable fit to solar neutrino data, if only or neutrino data alone are considered, but no allowed region is found in the combined analysis. Our results generalize to other neutrino-decay scenarios, including those that mediate when the neutrino mass ordering is inverted mass and , the mass of . Published by the American Physical Society2024 
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                            New constraints on oscillation parameters from νe appearance and νμ disappearance in the NOvA experiment
                        
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            The first results of the study of high-energy electron neutrino ( ) and muon neutrino ( ) charged-current interactions in the emulsion-tungsten detector of the FASER experiment at the LHC are presented. A 128.8 kg subset of the volume was analyzed after exposure to of data. Four (eight) ( ) interaction candidate events are observed with a statistical significance of ( ). This is the first direct observation of interactions at a particle collider and includes the highest-energy and ever detected from an artificial source. The interaction cross section per nucleon is measured over an energy range of 560–1740 GeV (520–1760 GeV) for ( ) to be [ ], consistent with standard model predictions. These are the first measurements of neutrino interaction cross sections in those energy ranges. Published by the American Physical Society2024more » « less
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