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@INPROCEEDINGS{Zavatarelli:838572,
author = {Zavatarelli, S. and Bellini, G. and Benziger, J. and Bick,
D. and Bonfini, G. and Bravo, D. and Caccianiga, B. and
Cadonati, L. and Calaprice, F. and Caminata, A. and
Cavalcante, P. and Chavarria, A. and Chepurnov, A. and
D'Angelo, D. and Davini, S. and Derbin, A. and Empl, A. and
Etenko, A. and Fomenko, K. and Franco, D. and Gabriele, F.
and Galbiati, C. and Gazzana, S. and Ghiano, C. and
Giammarchi, M. and Göger-Neff, M. and Goretti, A. and
Gromov, M. and Hagner, C. and Hungerford, E. and Ianni, Aldo
and Ianni, Andrea and Kobychev, V. and Korablev, D. and
Korga, G. and Kryn, D. and Laubenstein, M. and Lehnert, B.
and Lewke, T. and Litvinovich, E. and Lombardi, F. and
Lombardi, P. and Ludhova, L. and Lukyanchenko, G. and
Machulin, I. and Manecki, S. and Maneschg, W. and Marcocci,
S. and Meindl, Q. and Meroni, E. and Meyer, M. and
Miramonti, L. and Misiaszek, M. and Montuschi, M. and
Mosteiro, P. and Muratova, V. and Oberauer, L. and
Obolensky, M. and Ortica, F. and Otis, K. and Pallavicini,
M. and Papp, L. and Perasso, L. and Pocar, A. and Ranucci,
G. and Razeto, A. and Re, A. and Romani, A. and Rossi, N.
and Saldanha, R. and Salvo, C. and Schönert, S. and Simgen,
H. and Skorokhvatov, M. and Smirnov, O. and Sotnikov, A. and
Sukhotin, S. and Suvorov, Y. and Tartaglia, R. and Testera,
G. and Vignaud, D. and Vogelaar, R. B. and von Feilitzsch,
F. and Wang, H. and Winter, J. and Wojcik, M. and Wright, A.
and Wurm, M. and Zaimidoroga, O. and Zuber, K. and Zuzel,
G.},
title = {{R}ecent results from {B}orexino and the first real time
measure of solar pp neutrinos},
journal = {Nuclear and particle physics proceedings},
volume = {273-275},
issn = {2405-6014},
address = {Amsterdam [u.a.]},
publisher = {Elsevier},
reportid = {FZJ-2017-07154},
pages = {1753 - 1759},
year = {2016},
abstract = {The Borexino detector was built starting from 1996 in the
underground hall C of Gran Sasso National Laboratory (LNGS)
in Italy under about 1400 m of rock (3800 m.w.e) and it is
mostly aimed to the study in real-time of the low-energy
solar neutrinos.Since the beginning of data taking, in May
2007, the unprecedented detector radio-purity made the
performances of the detector unique: a milestone has been
very recently achieved with the measurement of solar pp
neutrino flux, providing the first direct observation in
real time of the key fusion reaction powering the Sun.In
this contribution the most important Borexino achievements
to the fields of solar, geo-neutrino and particle physics
are reviewed and the future perspectives discussed,
emphasizing in particular the unique possibility of Borexino
to cover at the end of its program the entire solar neutrino
spectrum and to exploit the possible existence of a fourth
sterile neutrino (SOX project).},
month = {Jul},
date = {2014-07-02},
organization = {37th International Conference on High
Energy Physics, Valencia (Spain), 2 Jul
2014 - 9 Jul 2014},
cin = {IKP-2},
ddc = {530},
cid = {I:(DE-Juel1)IKP-2-20111104},
pnm = {612 - Cosmic Matter in the Laboratory (POF3-612)},
pid = {G:(DE-HGF)POF3-612},
typ = {PUB:(DE-HGF)16 / PUB:(DE-HGF)8},
UT = {WOS:000390295200280},
doi = {10.1016/j.nuclphysbps.2015.09.282},
url = {https://juser.fz-juelich.de/record/838572},
}