'37 ar' presentation slideshows

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First Results from the Borexino Solar Neutrino Experiment

First Results from the Borexino Solar Neutrino Experiment. Celebrating F.Avignone, E.Fiorini & P. Rosen University of South Carolina May 16, 2008 Frank Calaprice. First Contact with Frank Avignone. 65 Zn source given by Ray Davis. Axion Searches Summary of Texono Coll. 2006. 65 Zn.

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1B11 Foundations of Astronomy The Sun

1B11 Foundations of Astronomy The Sun. Silvia Zane, Liz Puchnarewicz emp@mssl.ucl.ac.uk www.ucl.ac.uk/webct www.mssl.ucl.ac.uk/. 1B11 The Sun: a source of mystery to the human race. Newgrange, outside Dublin. Winter Solstice. 1B11 The Sun: a composite schematic illustration.

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1B11 Foundations of Astronomy The Sun

1B11 Foundations of Astronomy The Sun. Silvia Zane, Liz Puchnarewicz emp@mssl.ucl.ac.uk www.ucl.ac.uk/webct www.mssl.ucl.ac.uk/. 1B11 The Sun: a source of mystery to the human race. Newgrange, outside Dublin. Winter Solstice. 1B11 The Sun: a composite schematic illustration.

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Present status of the SAGE 37 Ar neutrino source experiment

Present status of the SAGE 37 Ar neutrino source experiment. PHYSICAL REVIEW C VOLUME 38, NUMBER 5 NOVEMBER 1988 37 Ar as a calibration source for solar neutrino detectors W.Haxton Institute for Nuclear Theory, Department of Physics,

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Solar neutrinos: form their production to their detection

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Solar neutrinos: form their production to their detection

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1962 Lederman,Schwartz,Steinberger Brookhaven National Laboratory

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Leptoni

Leptoni. Why 3 families? Are there more?. 2nd generation. 3rd generation. 2/3. 2/3. - 1/3. - 1/3. 0. 0. -1. -1. Fermions: the elementary players. The elementary particle families: fermions. 1st generation. Quarks. Leptons and quarks form doublets under weak interactions. Leptons.

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solar neutrino physics

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