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New limits on heavy sterile neutrino mixing in -decay obtained with the Borexino detector
Borexino collaboration, G. Bellini, J. Benziger +87
If heavy neutrinos with mass 2 are produced in the Sun via the decay in a side branch of pp-chain, they would…
Impact on Astrophysics and Elementary Particle Physics of recent and future solar neutrino data
Vito Antonelli, Lino Miramonti
The study of neutrinos is fundamental to connect astrophysics and elementary particle physics. In this last decade solar neutrino experiments and KamLAND confirmed the LMA solution…
Final results of Borexino Phase-I on low energy solar neutrino spectroscopy
Borexino Collaboration, G. Bellini, J. Benziger +87
Borexino has been running since May 2007 at the LNGS with the primary goal of detecting solar neutrinos. The detector, a large, unsegmented liquid scintillator calorimeter characte…
The Pierre Auger Observatory: Contributions to the 33rd International Cosmic Ray Conference (ICRC 2013)
The Pierre Auger Collaboration, Alexander Aab, Pedro Abreu +495
Contributions of the Pierre Auger Collaboration to the 33rd International Cosmic Ray Conference, Rio de Janeiro, Brazil, July 2013
SOX: Short distance neutrino Oscillations with BoreXino
Borexino Collaboration
The very low radioactive background of the Borexino detector, its large size, and the well proved capability to detect both low energy neutrino and anti-neutrino make an ideal case…
Advancements in solar neutrino physics
Vito Antonelli, Lino Miramonti
We review the results of solar neutrino physics, with particular attention to the data obtained and the analyses performed in the last decades, which were determinant to solve the…