Thanks to its extraordinary radiopurity, Borexino observed the two main fusion reactions in stars and will soon weigh in on a controversy relating to the birth of the Sun that challenges the SSM (G.Bellini & A.Ianni on CERN Courier)
Thesis
Jason Xavier Prochaska Senior Thesis. Princeton University, 1993 Michael Clinton Johnson PhD Thesis. Princeton University, 1998 Cristiano Galbiati PhD Thesis. University of Milano, 1999 Aldo Ianni PhD Thesis (Italian language). University of L’Aquila, 1999 Laura Cadonati PhD Thesis. Princeton University, 2000
Why and how the Sun and the stars shine
Borexino revealed for the first time the mechanisms powering the Sun and the other stars. In this article Prof. em. Gianpaolo Bellini describes the experiment and recollects its history and achievements (Il Nuovo Saggiatore Vol. 36, Anno 2020, No. 5-6, Pag. 82).
Testing the Scintillation Line Shape (Scaled Poisson)
Testing the Scintillation Line Shape (Scaled Poisson) – Oleg Ju. Smirnov
Response to the critics of Borexino results on electron stability
Response to the critics of Borexino results in “A New experimental limit for the stability of the electron” by H.V. Klapdor-Kleingrothaus, I.V. Krivosheina and I.V. Titkova
Borexino: Proposal for a low energy solar neutrino detector
Detailed Proposal for the Borexino experiment at LNGS, a real time detector for low energy solar neutrino, by G. Bellini, R. S. Raghavan et al.