Neutrinos, being the only fermions in the Standard Model of Particle Physics that do not
possess electromagnetic or color charges, have the unique opportunity to communicate with …

Since its original postulation by Wolfgang Pauli in 1930, the neutrino has played a
prominent role in our understanding of nuclear and particle physics. In the intervening 80 …

A bstract We discuss the possibility to explain the anomalies in short-baseline neutrino
oscillation experiments in terms of sterile neutrinos. We work in a 3+ 1 framework and pay …

This book accompanies another book by the same authors, Introduction to the Theory of the
Early Universe: Hot Big Bang Theory and presents the theory of the evolution of density …

The rate of neutrino-electron elastic scattering interactions from 862 keV Be 7 solar
neutrinos in Borexino is determined to be 46.0±1.5 (stat)-1.6+ 1.5 (syst) counts/(day· 100 …

A bstract Neutrino oscillations involving eV-scale neutrino mass states are investigated in
the context of global neutrino oscillation data including short and long-baseline accelerator …

The results of the third phase of the Super-Kamiokande solar neutrino measurement are
presented and compared to the first and second phase results. With improved detector …

A bstract We present an up-to-date global analysis of solar, atmospheric, reactor, and
accelerator neutrino data in the framework of three-neutrino oscillations. We provide results …

We report an improved measurement of the neutrino mixing angle θ 13 from the Daya Bay
Reactor Neutrino Experiment. We exclude a zero value for sin 2 2θ 13 with a significance of …

We observed, for the first time, solar neutrinos in the 1.0–1.5 MeV energy range. We
determined the rate of pep solar neutrino interactions in Borexino to be 3.1±0.6 stat±0.3 syst …