Results from Solar Neutrino Radiochemical Experiments (with main emphasis on Gallium) Neutrino 2004, Paris 13-18 June 2004 Carla Maria Cattadori INFN Milano.
1962 Lederman,Schwartz,Steinberger Brookhaven National Laboratory
NEUTRINO OSCILLATIONS Luigi DiLella Physics Dept. and INFN, Pisa, Italy
Telescopes: SNO and the New SNOLAB Art McDonald Queen’s University, Kingston For the SNO Collaboration 2 km underground in Vale-INCO’s Creighton Mine near.
1 Primordial nucleosynthesis and New Physics Maxim Pospelov University of Victoria and Perimeter Institute K. Jedamzik and M. Pospelov, arXiv:0906.2087.
NEUTRINO OSCILLATIONS Luigi DiLella Physics Dept. and INFN, Pisa, Italy CHIPP PhD Winter School 2011 Formalism of neutrino oscillations in vacuum Solar.
GEANT4 simulation of the Borexino solar neutrino experiment. Igor Machulin Moscow, Kurchatov Institute On behalf of the Borexino Collaboration Catania,
Adam Para 1. Or rather Stories about neutrino detection.
( E ) = S(E) e –2 E -1 2 m m m m Reaction Rate(star) (E) (E) dE Gamow Peak Maxwell Boltzmann.
Yuri Kamyshkov/ University of Tennessee email: kamyshkov@utk
K. Jedamzik and M . Pospelov, arXiv:0906.2087 R. Cyburt and M. Pospelov, arXiv:0906.4373
J. Pradler and M.Pospelov , to appear ~ next weak