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What can we learn on supernova neutrino spectra with water Cherenkov detectors?
Andrea Gallo Rosso, Francesco Vissani, Maria Cristina Volpe
We investigate the precision with which the supernova neutrino spectra can be reconstructed in water Cherenkov detectors, in particular the large scale Hyper-Kamiokande and Super-K…
Testing creation of matter with neutrinoless double beta decay
Stefano Dell'Oro, Simone Marcocci, Francesco Vissani
In this brief review, the importance of the so called neutrinoless double beta decay transition in the search for physics beyond the Standard Model is emphasized. The expectations…
Joint analysis of Borexino and SNO solar neutrino data and reconstruction of the survival probability
Francesco Vissani
Solar neutrino oscillations are supported by KamLAND's antineutrino measurements, but certain solar neutrino data - the observed shape of the B flux and the difference betwee…
On the compatibility of the IceCube results with an universal neutrino spectrum
Andrea Palladino, Carlo Mascaretti, Francesco Vissani
There is mounting evidence that the IceCube findings cannot be described simply invoking a single power-law spectrum for cosmic neutrinos. We discuss which are the minimal modifica…
Measuring the neutron star compactness and binding energy with supernova neutrinos
Andrea Gallo Rosso, Francesco Vissani, Maria Cristina Volpe
We investigate the precision with which a neutron star gravitational binding energy can be measured through the supernova neutrino signal, without assuming any prior such as the en…
Solar neutrino physics on the beginning of 2017
Francesco Vissani
This writeup is a review of current hot topics on solar neutrinos. It is based on a talk at the conference "Neutrinos: the quest for a new physics scale", held at the CERN on March…