A plausible explanation for the lightness of neutrino masses is that neutrinos are massless at
tree level, with their mass (typically Majorana) being generated radiatively at one or more …

We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting
views and insights from all disciplines involved-cosmology, astrophysics, nuclear, and …

Abstract The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose
underground liquid scintillator detector, was proposed with the determination of the neutrino …

Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the
infall dynamics of the stellar core, triggering and fueling the explosion and driving the …

A measurement of electron antineutrino oscillation by the Daya Bay Reactor Neutrino
Experiment is described in detail. Six 2.9-GWth nuclear power reactors of the Daya Bay and …

A bstract The Double Chooz experiment presents improved measurements of the neutrino
mixing angle θ 13 using the data collected in 467.90 live days from a detector positioned at …

We present cosmological results from the final galaxy clustering data set of the Baryon
Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined …

Here, we update our previous global fit of neutrino oscillations by including the recent results
that have appeared since the Neutrino 2012 conference. These include the measurements …

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 …

Hyper-Kamiokande will be a next-generation underground water Cherenkov detector with a
total (fiducial) mass of 0.99 (0.56) million metric tons, approximately 20 (25) times larger than …