A number of anomalous results in short-baseline oscillation may hint at the existence of one
or more light sterile neutrino states in the eV mass range and have triggered a wave of new …

Neutrinos are the only particles in the Standard Model that could be Majorana fermions, that
is, completely neutral fermions that are their own antiparticles. The most sensitive known …

For most of their existence, stars are fuelled by the fusion of hydrogen into helium. Fusion
proceeds via two processes that are well understood theoretically: the proton–proton (pp) …

We propose the construction of LEGEND-1000, the ton-scale Large Enriched Germanium
Experiment for Neutrinoless $\beta\beta $ Decay. This international experiment is designed …

Building on the successful experience in operating the DarkSide-50 detector, the DarkSide
Collaboration is going to construct DarkSide-20k, a direct WIMP search detector using a two …

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

About 99 per cent of solar energy is produced through sequences of nuclear reactions that
convert hydrogen into helium, starting from the fusion of two protons (the pp chain). The …

The Sudbury Neutrino Observatory (SNO) experiment [1] took data from 1999 to 2006,
before returning its target heavy water (2H2O or D2O) to the supplier. Using much of the …

The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a-
generation opportunity to obtain detailed information about the explosion of a star and …

In the core of the Sun, energy is released through sequences of nuclear reactions that
convert hydrogen into helium. The primary reaction is thought to be the fusion of two protons …