Results 1 to 10 of about 5,547 (200)
Solar neutrino with Borexino: Results and perspectives [PDF]
Physics of Particles and Nuclei, 2015 Borexino is a unique detector able to perform measurement of solar neutrinos
fluxes in the energy region around 1 MeV or below due to its low level of
radioactive background. It was constructed at the LNGS underground laboratory
with a goal of solar $^{7}O. Smirnov, G. Bellini, J. Benziger, D. Bick, G. Bonfini, D. Bravo, B. Caccianiga, F. Calaprice, A. Caminata, P. Cavalcante, Á. Chavarría, A. Chepurnov, D. D’Angelo, S. Davini, A. Derbin, A. Empl, A. Etenko, K. Fomenko, D. Franco, G. Fiorentini, C. Galbiati, S. Gazzana, C. Ghiano, M. Giammarchi, M. Göger‐Neff, A. Goretti, C. Hagner, E. Hungerford, Aldo Ianni, Andrea Ianni, V. Kobychev, D. Korablëv, G. Korga, D. Kryn, M. Laubenstein, B. Lehnert, T. Lewke, E. Litvinovich, F. Lombardi, P. Lombardi, L. Ludhová, G. Lukyanchenko, I. Machulin, S. Manecki, W. Maneschg, Fabio Mantovani, S. Marcocci, Q. Meindl, E. Meroni, M. Meyer, L. Miramonti, M. Misiaszek, P. Mosteiro, V. Muratova, L. Oberauer, M. Obolensky, F. Ortica, K. Otis, M. Pallavicini, L. Papp, L. Perasso, A. Pocar, G. Ranucci, A. Razeto, A. Re, B. Ricci, A. Romani, N. Rossi, R. Saldanha, C. Salvo, S. Schönert, H. Simgen, M. Skorokhvatov, A. Sotnikov, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, D. Vignaud, R.B. Vogelaar, F. von Feilitzsch, H. Wang, J. Winter, M. Wójcik, A. Wright, M. Wurm, O. Zaimidoroga, S. Zavatarelli, Κ. Zuber, G. Zuzel +89 morecore +14 more sourcesBorexino calibrations: hardware, methods, and results [PDF]
Journal of Instrumentation, 2012 Borexino was the first experiment to detect solar neutrinos in real-time in
the sub-MeV region. In order to achieve high precision in the determination of
neutrino rates, the detector design includes an internal and an external
calibration system.H. Back, G Bellini, J Benziger, D. Bick, G. Bonfini, D. Bravo, M. Buizza Avanzini, B. Caccianiga, L. Cadonati, F. Calaprice, C. Carraro, P. Cavalcante, A. Chavarria, A. Chepurnov, D D\textquoteright Angelo, S. Davini, A Derbin, A. Etenko, F. von Feilitzsch, G. Fernandes, K Fomenko, D. Franco, C Galbiati, S. Gazzana, C. Ghiano, M. Giammarchi, M. Goeger-Neff, A. Goretti, L. Grandi, E. Guardincerri, Hardy S, Aldo Ianni, Andrea Ianni, A. Kayunov, S. Kidner, V. Kobychev, D. Korablev, G. Korga, Y Koshio, D. Kryn, M Laubenstein, T. Lewke, E Litvinovich, Ben Loer, F. Lombardi, P. Lombardi, L. Ludhova, I Machulin, S. Manecki, W. Maneschg, G. Manuzio, Q. Meindl, E. Meroni, L. Miramonti, M. Misiaszek, D. Montanari, P. Mosteiro, V. Muratova, L. Oberauer, M. Obolensky, F. Ortica, K. Otis, M. Pallavicini, L. Papp, L. Perasso, S Perasso, A. Pocar, R. S. Raghavan, Ranucci G, A. Razeto, Re A, A Romani, Rossi N, D. Rountree, A Sabelnikov, R. Saldanha, C. Salvo, S. Schönert, H. Simgen, M. Skorokhvatov, O. Smirnov, A. Sotnikov, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, D. Vignaud, R.B. Vogelaar, J. Winter, M. Wojcik, A. Wright, M. Wurm, J. Xu, O. Zaimidoroga, S. Zavatarelli, G. Zuzel, H. Back, G Bellini, J Benziger, D. Bick +99 morecore +7 more sourcesIdentification of the cosmogenic $$^{11}$$ 11 C background in large volumes of liquid scintillators with Borexino
European Physical Journal C: Particles and Fields, 2021 Cosmogenic radio-nuclei are an important source of background for low-energy neutrino experiments. In Borexino, cosmogenic $$^{11}$$ 11 C decays outnumber solar pep and CNO neutrino events by about ten to one.M. Agostini, K. Altenmüller, S. Appel, V. Atroshchenko, Z. Bagdasarian, D. Basilico, G. Bellini, J. Benziger, R. Biondi, D. Bravo, B. Caccianiga, F. Calaprice, A. Caminata, P. Cavalcante, A. Chepurnov, D. D’Angelo, S. Davini, A. Derbin, A. Di ZGiacintio, V. Di Marcello, X. F. Ding, A. Di Ludovico, L. Di Noto, I. Drachnev, A. Formozov, D. Franco, C. Galbiati, C. Ghiano, M. Giammarchi, A. Goretti, A. S. Göttel, M. Gromov, D. Guffanti, Aldo Ianni, Andrea Ianni, A. Jany, D. Jeschke, V. Kobychev, G. Korga, S. Kumaran, M. Laubenstein, E. Litvinovich, P. Lombardi, I. Lomskaya, L. Ludhova, G. Lukyanchenko, L. Lukyanchenko, I. Machulin, J. Martyn, E. Meroni, M. Meyer, L. Miramonti, M. Misiaszek, V. Muratova, B. Neumair, M. Nieslony, R. Nugmanov, L. Oberauer, V. Orekhov, F. Ortica, M. Pallavicini, L. Papp, L. Pelicci, Ö. Penek, L. Pietrofaccia, N. Pilipenko, A. Pocar, A. Porcelli, G. Raikov, M. T. Ranalli, G. Ranucci, A. Razeto, A. Re, M. Redchuk, A. Romani, N. Rossi, S. Schönert, D. Semenov, G. Settanta, M. Skorokhvatov, A. Singhal, O. Smirnov, A. Sotnikov, Y. Suvorov, R. Tartaglia, G. Testera, J. Thurn, E. Unzhakov, A. Vishneva, R. B. Vogelaar, F. von Feilitzsch, M. Wojcik, M. Wurm, S. Zavatarelli, K. Zuber, G. Zuzel +95 moredoaj +3 more sourcesNew limits on heavy sterile neutrino mixing inB8decay obtained with the Borexino detector [PDF]
, 2013 If heavy neutrinos with mass $m_{\nu_{H}}\geq$2$ m_e $ are produced in the
Sun via the decay ${^8\rm{B}} \rightarrow {^8\rm{Be}} + e^+ + \nu_H$ in a side
branch of pp-chain, they would undergo the observable decay into an electron, a
positron and a light G. Bellini, J. Benziger, D. Bick, G. Bonfini, D. Bravo, M. Buizza Avanzini, B. Caccianiga, L. Cadonati, F. Calaprice, P. Cavalcante, Á. Chavarría, A. Chepurnov, D. D’Angelo, S. Davini, A. Derbin, I. Drachnev, A. Empl, A. Etenko, K. Fomenko, D. Franco, C. Galbiati, S. Gazzana, C. Ghiano, M. Giammarchi, M. Göger‐Neff, A. Goretti, L. Grandi, C. Hagner, E. Hungerford, Aldo Ianni, Andrea Ianni, V. Kobychev, D. Korablëv, G. Korga, D. Kryn, M. Laubenstein, T. Lewke, E. Litvinovich, B. Loer, F. Lombardi, P. Lombardi, L. Ludhová, G. Lukyanchenko, I. Machulin, S. Manecki, W. Maneschg, G. Manuzio, Q. Meindl, E. Meroni, L. Miramonti, M. Misiaszek, P. Mosteiro, V. Muratova, L. Oberauer, M. Obolensky, F. Ortica, K. Otis, M. Pallavicini, L. Papp, L. Perasso, S. Perasso, A. Pocar, G. Ranucci, A. Razeto, A. Re, A. Romani, N. Rossi, R. Saldanha, C. Salvo, S. Schönert, H. Simgen, M. Skorokhvatov, O. Smirnov, A. Sotnikov, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, D. Vignaud, R. B. Vogelaar, F. von Feilitzsch, J. Winter, M. Wójcik, A. Wright, M. Wurm, Jing Xu, O. Zaimidoroga, S. Zavatarelli, G. Zuzel +88 moreopenalex +5 more sourcesShort distance neutrino oscillations with Borexino [PDF]
EPJ Web of Conferences, 2016 The Borexino detector has convincingly shown its outstanding performances in the low energy, sub-MeV regime through its unprecedented accomplishments in the solar and geo-neutrinos detection.Caminata A., Agostini M., Altenmüller K., Appel S., Bellini G., Benziger J., Berton N., Bick D., Bonfini G., Bravo D., Caccianiga B., Calaprice F., Cavalcante P., Chepurnov A., Cribier M., D'Angelo D., Davini S., Derbin A., Noto L. di, Durero M., Empl A., Etenko A., Farinon S., Fischer V., Fomenko K., Franco D., Gabriele F., Gaffiot J., Galbiati C., Ghiano C., Giammarchi M., Göger-Neff M., Goretti A., Gromov M., Hagner C., Houdy Th., Hungerford E., Ianni Aldo, Ianni Andrea, Jonquères N., Kaiser M., Kobychev V., Korablev D., Korga G., Kryn D., Lachenmaier T., Lasserre T., Laubenstein M., Lehnert B., Link J., Litvinovich E., Lombardi F., Lombardi P., Ludhova L., Lukyanchenko G., Machulin I., Maneschg W., Marcocci S., Maricic J., Mention G., Meroni E., Meyer M., Miramonti L., Misiaszek M., Montuschi M., Muratova V., Musenich R., Neumair B., Oberauer L., Obolensky M., Ortica F., Pallavicini M., Papp L., Perasso L., Pocar A., Ranucci G., Razeto A., Re A., Romani A., Rossi N., Schönert S., Scola L., Simgen H., Skorokhvatov M., Smirnov O., Sotnikov A., Sukhotin S., Suvorov Y., Tartaglia R., Testera G., Veyssière C., Vivier M., Vogelaar R.B., Feilitzsch F. von, Wang H., Winter J., Wojcik M., Wurm M., Zaimidoroga O., Zavatarelli S., Zuber K., Zuzel G. +101 moredoaj +2 more sourcesThe Borexino Thermal Monitoring & Management System and simulations of the fluid-dynamics of the Borexino detector under asymmetrical, changing boundary conditions [PDF]
, 2017 A comprehensive monitoring system for the thermal environment inside the
Borexino neutrino detector was developed and installed in order to reduce
uncertainties in determining temperatures throughout the detector.D. Bravo, Riccardo Mereu, P. Cavalcante, M. Carlini, Aldo Ianni, A. Goretti, F. Gabriele, T. Wright, Z. Yokley, R. B. Vogelaar, F. Calaprice, Fabio Inzoli +11 moreopenalex +3 more sourcesThe nylon scintillator containment vessels for the Borexino solar neutrino experiment [PDF]
, 2007 Borexino is a solar neutrino experiment designed to observe the 0.86 MeV Be-7
neutrinos emitted in the pp cycle of the sun. Neutrinos will be detected by
their elastic scattering on electrons in 100 tons of liquid scintillator. The
neutrino event rate in Jay B. Benziger, L. Cadonati, F. Calaprice, E. de Haas, Robert Fernholz, R. Ford, C. Galbiati, A. Goretti, Eric Harding, Aldo Ianni, An. Ianni, S. Kidner, M. Leung, F. Loeser, K. McCarty, A. Nelson, R. Parsells, A. Pocar, T. Shutt, A. Sonnenschein, R. B. Vogelaar +20 moreopenalex +5 more sources
