What is the origin of the oxygen we breathe, the hydrogen and oxygen (in form of water
H2O) in rivers and oceans, the carbon in all organic compounds, the silicon in electronic …

The available data on nuclear fusion cross sections important to energy generation in the
Sun and other hydrogen-burning stars and to solar neutrino production are summarized and …

The Review summarizes much of particle physics and cosmology. Using data from previous
editions, plus 2,873 new measurements from 758 papers, we list, evaluate, and average …

This is the first of a series of papers presenting the Modules for Experiments in Stellar
Astrophysics (MESA) Isochrones and Stellar Tracks (MIST) project, a new comprehensive …

We compute a new generation of standard solar models (SSMs) that includes recent
updates on some important nuclear reaction rates and a more consistent treatment of 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 …

We present a re-analysis of the Geneva-Copenhagen survey, which benefits from the
infrared flux method to improve the accuracy of the derived stellar effective temperatures and …

This biennial Review summarizes much of particle physics. Using data from previous
editions, plus 2158 new measurements from 551 papers, we list, evaluate, and average …

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 …

Borexino has been running since May 2007 at the Laboratori Nazionali del Gran Sasso
laboratory in Italy with the primary goal of detecting solar neutrinos. The detector, a large …