
doi: 10.22323/1.084.0277
Marian Smoluchowski Institute of PhysicsJagiellonian Universityul. Reymonta 4, 30-059 Krakow, PolandE-mail:marcin.misiaszek@uj.edu.plOn Behalf of the Borexino Collaboration:C. Arpesella, H. O. Back, M. Balata, G. Bellini, J. Benziger, S. Bonetti, A. Brigatti, B.Caccianiga, L. Cadonati, F. Calaprice, C. Carraro, G. Cecchet, A. Chavarria, M. Chen, F.Dalnoki-Veress, D. DAngelo, A. de Bari, A. de Bellefon, H. deKerret, A. Derbin, M. Deutsch, A.di Credico, G. di Pietro, R. Eisenstein, F. Elisei, A. Etenko, R. Fernholz, K. Fomenko, R. Ford, D.Franco, B. Freudiger, C. Galbiati, F. Gatti, S. Gazzana, M. Giammarchi, D. Giugni, M.Goeger-Neff, T. Goldbrunner, A. Goretti, C. Grieb, C. Hagner, W. Hampel, E. Harding, S. Hardy,F. X. Hartman, T. Hertrich, G. Heusser, Aldo Ianni, Andrea Ianni, M. Joyce, J. Kiko, T. Kirsten,V. Kobychev, G. Korga, G. Korschinek, D. Kryn, V. Lagomarsino, P. Lamarche, M. Laubenstein,C. Lendvai, M. Leung, T. Lewke, E. Litvinovich, B. Loer, P. Lombardi, L. Ludhova, I. Machulin,S. Malvezzi, S. Manecki, J. Maneira, W. Maneschg, I. Manno, D. Manuzio, G. Manuzio, A.Martemianov, F. Masetti, U. Mazzucato, K. McCarty, D. McKinsey, Q. Meindl, E. Meroni, L.Miramonti, D. Montanari, M. E. Monzani, V. Muratova, P. Musico, H. Neder, A. Nelson, L.Niedermeier, L. Oberauer, M. Obolensky, M. Orsini, F. Ortica, M. Pallavicini, L. Papp, S.Parmeggiano, L. Perasso, A. Pocar, R. S. Raghavan, G. Ranucci, W. Rau, A. Razeto, E. Resconi,P. Risso, A. Romani, D. Rountree, A. Sabelnikov, R. Saldanha, C. Salvo, D. Schimizzi, S.SchAu˝nert, T. Shutt, H. Simgen, M. Skorokhvatov, O. Smirnov, A. Sonnenschein, A. Sotnikov, S.Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, D. Vignaud, S. Vitale, R. B. Vogelaar, F. vonFeilitzsch, R. von Hentig, T. von Hentig, M. Wojcik, M. Wurm, O. Zaimidoroga, S. Zavatarelliand G. ZuzelBorexino is a large-volume liquid scintillator detector placed in the underground halls of the Lab-oratori Nazionali del Gran Sasso in Italy. It is able to detect in real time neutrino interactionsbelow 2 MeV, due to the very high radio-purity reached by the detector. The interaction rate ofthe 0.862 MeV
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 1 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
