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) …

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 …

We present updated results from the NOvA experiment for ν μ→ ν μ and ν μ→ ν e oscillations
from an exposure of 8.85× 10 20 protons on target, which represents an increase of 46 …

We revisit the physics of neutrino magnetic moments, focusing in particular on the case
where the right-handed, or sterile, neutrinos are heavier (up to several MeV) than the left …

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 …

We present the simultaneous measurement of the interaction rates R pp, R Be, R pep of pp,
Be 7, and pep solar neutrinos performed with a global fit to the Borexino data in an extended …

This paper presents a comprehensive geoneutrino measurement using the Borexino
detector, located at Laboratori Nazionali del Gran Sasso (LNGS) in Italy. The analysis is the …

A bstract We present a detailed analysis of the spectral data of Borexino Phase II, with the
aim of exploiting its full potential to constrain scenarios beyond the Standard Model. In …

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 …

Borexino is a 280-ton liquid scintillator detector located at the Laboratori Nazionali del Gran
Sasso in Italy. Since the start of its data-taking in May 2007, it has provided several …