In this article we review the current state of the field of solar neutrinos, including flavor
oscillations, nonstandard effects, solar models, cross section measurements, and the broad …

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 present an improved measurement of the carbon-nitrogen-oxygen (CNO) solar neutrino
interaction rate at Earth obtained with the complete Borexino Phase-III dataset. The …

The fundamental processes by which nuclear energy is generated in the Sun have been
known for many years. However, continuous progress in areas such as neutrino …

In this paper, we report the first measurement of CNO solar neutrinos by Borexino that uses
the correlated integrated directionality (CID) method, exploiting the subdominant Cherenkov …

We report the measurement of sub-MeV solar neutrinos through the use of their associated
Cherenkov radiation, performed with the Borexino detector at the Laboratori Nazionali del …

In this paper, we find that a magnetic transition dipole moment between tau and sterile
neutrinos can account for the XENON1T excess events. Unlike the ordinary neutrino dipole …

This paper presents studies of the performance of water-based liquid scintillators (WbLS) in
both 1-kt and 50-kt detectors. Performance is evaluated in comparison to both pure water …

Liquid scintillator detectors play a central role in the detection of neutrinos from various
sources. In particular, it is the only technique used so far for the precision spectroscopy of …

It is still unknown whether the mass terms for neutrinos are of Majorana type or of Dirac type.
An interesting possibility, known as pseudo-Dirac scheme, combines these two with a …