Science and technology of Borexino: A real-time detector for low energy solar neutrinos

G. Alimonti; C. Arpesella; H. Back; M. Balata; T. Beau; G. Bellini; J. Benziger; S. Bonetti; A. Brigatti; B. Caccianiga; L. Cadonati; F. Calaprice; G. Cecchet; M. Chen; A. DeBari; E. DeHaas; H. De Kerret; O. Donghi; M. Deutsch; F. Elisei; A. Etenko; F. Von Feilitzsch; R. Fernholz; R. Ford; B. Freudiger; A. Garagiola; C. Galbiati; F. Gatti; S. Gazzana; M. Giammarchi; D. Giugni; A. Golubchikov; A. Goretti; C. Grieb; C. Hagner; T. Hagner; W. Hampel; E. Harding; F. Hartmann; R. Von Hentig; H. Hess; G. Heusser; A. Ianni; P. Inzani; S. Kidner; J. Kiko; T. Kirsten; G. Korga; G. Korschinek; D. Kryn; V. Lagomarsino; P. LaMarcne; M. Laubenstein; F. Loeser; P. Lombardi; S. Magni; S. Malvezzi; J. Maniera; I. Manno; G. Manuzio; F. Masetti; U. Mazzucato; E. Meroni; P. Musico; H. Neder; M. Neff; S. Nisi; L. Oberauer; M. Obolensky; M. Pallavicini; L. Papp; L. Perasso; A. Pocar; R. Raghavan; G. Ranucci; W. Rau; A. Razeto; E. Resconi; T. Riedel; A. Sabelnikov; P. Saggese; C. Salvo; R. Scardaoni; S. Schoenert; K. Schuhbeck; H. Seidel; T. Shutt; H. Simgen; A. Sonnenschein; O. Smirnov; A. Sotnikov; M. Skorokhvatov; S. Sukhotin; R. Tartaglia; G. Testera; R. Vogelaar; S. Vitale; M. Wojcik; O. Zaimidoroga; Y. Zakharov

doi:10.1016/S0927-6505(01)00110-4

Science and technology of Borexino: A real-time detector for low energy solar neutrinos

G. Alimonti
, C. Arpesella
, H. Back
, M. Balata
, T. Beau
, G. Bellini
, J. Benziger
, S. Bonetti
, A. Brigatti
, B. Caccianiga
, L. Cadonati
, F. Calaprice
, G. Cecchet
, M. Chen
, A. DeBari
, E. DeHaas
, H. De Kerret
, O. Donghi
, M. Deutsch
, F. Elisei

A. Etenko, F. Von Feilitzsch, R. Fernholz, R. Ford, B. Freudiger, A. Garagiola, C. Galbiati, F. Gatti, S. Gazzana, M. Giammarchi, D. Giugni, A. Golubchikov, A. Goretti, C. Grieb, C. Hagner, T. Hagner, W. Hampel, E. Harding, F. Hartmann, R. Von Hentig, H. Hess, G. Heusser, A. Ianni, P. Inzani, S. Kidner, J. Kiko, T. Kirsten, G. Korga, G. Korschinek, D. Kryn, V. Lagomarsino, P. LaMarcne, M. Laubenstein, F. Loeser, P. Lombardi, S. Magni, S. Malvezzi, J. Maniera, I. Manno, G. Manuzio, F. Masetti, U. Mazzucato, E. Meroni, P. Musico, H. Neder, M. Neff, S. Nisi, L. Oberauer, M. Obolensky, M. Pallavicini, L. Papp, L. Perasso, A. Pocar, R. Raghavan, G. Ranucci, W. Rau, A. Razeto, E. Resconi, T. Riedel, A. Sabelnikov, P. Saggese, C. Salvo, R. Scardaoni, S. Schoenert, K. Schuhbeck, H. Seidel, T. Shutt, H. Simgen, A. Sonnenschein, O. Smirnov, A. Sotnikov, M. Skorokhvatov, S. Sukhotin, R. Tartaglia, G. Testera, R. Vogelaar, S. Vitale, M. Wojcik, O. Zaimidoroga, Y. Zakharov

Research output: Contribution to journal › Article › peer-review

301 Scopus citations

Abstract

Borexino, a real-time device for low energy neutrino spectroscopy is nearing completion of construction in the underground laboratories at Gran Sasso, Italy (LNGS). The experiment's goal is the direct measurement of the flux of ⁷Be solar neutrinos of all flavors via neutrino-electron scattering in an ultra-pure scintillation liquid. Seeded by a series of innovations which were brought to fruition by large-scale operation of a 4-ton test detector at LNGS, a new technology has been developed for Borexino. It enables sub-MeV solar neutrino spectroscopy for the first time. This paper describes the design of Borexino, the various facilities essential to its operation, its spectroscopic and background suppression capabilities and a prognosis of the impact of its results towards resolving the solar neutrino problem. Borexino will also address several other frontier questions in particle physics, astrophysics and geophysics.

Original language	English
Pages (from-to)	205-234
Number of pages	30
Journal	Astroparticle Physics
Volume	16
Issue number	3
DOIs	https://doi.org/10.1016/S0927-6505(01)00110-4
State	Published - Jan 2002
Externally published	Yes

Bibliographical note

Funding Information:
Many individuals besides the authors have contributed to the development of the Borexino project. We wish to acknowledge particularly the following who made significant contributions in early stages: R. Cereseto, N. Darnton, A. Falgiani, T. Goldbrunner, J. Jochum, M. Johnson, A. Manco, A. Nostro, S. Pakvasa, M. Parodi, A. Perotti, G. Pieri, A. Preda, P. Raghavan, P. Rothschild, P. Ullucci and members of IRMM for the measurements made in Geel. The collaboration wants to thank the Laboratori Nazionali del Gran Sasso [LNGS] and A. Bettini for continuous help and support. We sincerely thank the funding bodies: Istituto Nazionale di Fisica Nucleare [INFN], and Ministero della Universita' e della Ricerca Scientifica e Tecnologica [MURST] (Italy); IN2P3 (France); Bundesministerium für Bildung, Wissenschaft, Forschung und Technologie [BMBF], Deutsche Forschungsgemeinschaft [DFG] and Max-Planck-Gesellschaft [MPG] (Germany); the National Science Foundation and Bell Laboratories (USA); the Natural Sciences and Engineering Research Council of Canada, and agencies in Hungary, Poland and Russia for their generous support of this project.

Funding

Many individuals besides the authors have contributed to the development of the Borexino project. We wish to acknowledge particularly the following who made significant contributions in early stages: R. Cereseto, N. Darnton, A. Falgiani, T. Goldbrunner, J. Jochum, M. Johnson, A. Manco, A. Nostro, S. Pakvasa, M. Parodi, A. Perotti, G. Pieri, A. Preda, P. Raghavan, P. Rothschild, P. Ullucci and members of IRMM for the measurements made in Geel. The collaboration wants to thank the Laboratori Nazionali del Gran Sasso [LNGS] and A. Bettini for continuous help and support. We sincerely thank the funding bodies: Istituto Nazionale di Fisica Nucleare [INFN], and Ministero della Universita' e della Ricerca Scientifica e Tecnologica [MURST] (Italy); IN2P3 (France); Bundesministerium für Bildung, Wissenschaft, Forschung und Technologie [BMBF], Deutsche Forschungsgemeinschaft [DFG] and Max-Planck-Gesellschaft [MPG] (Germany); the National Science Foundation and Bell Laboratories (USA); the Natural Sciences and Engineering Research Council of Canada, and agencies in Hungary, Poland and Russia for their generous support of this project.

Funders
Bell Laboratories
MURST
National Science Foundation
Natural Sciences and Engineering Research Council of Canada
Deutsche Forschungsgemeinschaft
Bundesministerium für Bildung und Forschung
Instituto Nazionale di Fisica Nucleare
Max-Planck-Gesellschaft
Ministero dell'Ambiente e della Tutela del Territorio e del Mare
Bundesministerium für Bildung, Wissenschaft, Forschung und Technologie
Institut national de physique nucléaire et de physique des particules
Istituto Nazionale di Fisica Nucleare

Access to Document

10.1016/S0927-6505(01)00110-4

Cite this

Alimonti, G., Arpesella, C., Back, H., Balata, M., Beau, T., Bellini, G., Benziger, J., Bonetti, S., Brigatti, A., Caccianiga, B., Cadonati, L., Calaprice, F., Cecchet, G., Chen, M., DeBari, A., DeHaas, E., De Kerret, H., Donghi, O., Deutsch, M., ... Zakharov, Y. (2002). Science and technology of Borexino: A real-time detector for low energy solar neutrinos. Astroparticle Physics, 16(3), 205-234. https://doi.org/10.1016/S0927-6505(01)00110-4

@article{6027787330ff4e90a3fe4212ca35403c,

title = "Science and technology of Borexino: A real-time detector for low energy solar neutrinos",

abstract = "Borexino, a real-time device for low energy neutrino spectroscopy is nearing completion of construction in the underground laboratories at Gran Sasso, Italy (LNGS). The experiment's goal is the direct measurement of the flux of 7Be solar neutrinos of all flavors via neutrino-electron scattering in an ultra-pure scintillation liquid. Seeded by a series of innovations which were brought to fruition by large-scale operation of a 4-ton test detector at LNGS, a new technology has been developed for Borexino. It enables sub-MeV solar neutrino spectroscopy for the first time. This paper describes the design of Borexino, the various facilities essential to its operation, its spectroscopic and background suppression capabilities and a prognosis of the impact of its results towards resolving the solar neutrino problem. Borexino will also address several other frontier questions in particle physics, astrophysics and geophysics.",

author = "G. Alimonti and C. Arpesella and H. Back and M. Balata and T. Beau and G. Bellini and J. Benziger and S. Bonetti and A. Brigatti and B. Caccianiga and L. Cadonati and F. Calaprice and G. Cecchet and M. Chen and A. DeBari and E. DeHaas and \{De Kerret\}, H. and O. Donghi and M. Deutsch and F. Elisei and A. Etenko and \{Von Feilitzsch\}, F. and R. Fernholz and R. Ford and B. Freudiger and A. Garagiola and C. Galbiati and F. Gatti and S. Gazzana and M. Giammarchi and D. Giugni and A. Golubchikov and A. Goretti and C. Grieb and C. Hagner and T. Hagner and W. Hampel and E. Harding and F. Hartmann and \{Von Hentig\}, R. and H. Hess and G. Heusser and A. Ianni and P. Inzani and S. Kidner and J. Kiko and T. Kirsten and G. Korga and G. Korschinek and D. Kryn and V. Lagomarsino and P. LaMarcne and M. Laubenstein and F. Loeser and P. Lombardi and S. Magni and S. Malvezzi and J. Maniera and I. Manno and G. Manuzio and F. Masetti and U. Mazzucato and E. Meroni and P. Musico and H. Neder and M. Neff and S. Nisi and L. Oberauer and M. Obolensky and M. Pallavicini and L. Papp and L. Perasso and A. Pocar and R. Raghavan and G. Ranucci and W. Rau and A. Razeto and E. Resconi and T. Riedel and A. Sabelnikov and P. Saggese and C. Salvo and R. Scardaoni and S. Schoenert and K. Schuhbeck and H. Seidel and T. Shutt and H. Simgen and A. Sonnenschein and O. Smirnov and A. Sotnikov and M. Skorokhvatov and S. Sukhotin and R. Tartaglia and G. Testera and R. Vogelaar and S. Vitale and M. Wojcik and O. Zaimidoroga and Y. Zakharov",

note = "Funding Information: Many individuals besides the authors have contributed to the development of the Borexino project. We wish to acknowledge particularly the following who made significant contributions in early stages: R. Cereseto, N. Darnton, A. Falgiani, T. Goldbrunner, J. Jochum, M. Johnson, A. Manco, A. Nostro, S. Pakvasa, M. Parodi, A. Perotti, G. Pieri, A. Preda, P. Raghavan, P. Rothschild, P. Ullucci and members of IRMM for the measurements made in Geel. The collaboration wants to thank the Laboratori Nazionali del Gran Sasso [LNGS] and A. Bettini for continuous help and support. We sincerely thank the funding bodies: Istituto Nazionale di Fisica Nucleare [INFN], and Ministero della Universita' e della Ricerca Scientifica e Tecnologica [MURST] (Italy); IN2P3 (France); Bundesministerium f{\"u}r Bildung, Wissenschaft, Forschung und Technologie [BMBF], Deutsche Forschungsgemeinschaft [DFG] and Max-Planck-Gesellschaft [MPG] (Germany); the National Science Foundation and Bell Laboratories (USA); the Natural Sciences and Engineering Research Council of Canada, and agencies in Hungary, Poland and Russia for their generous support of this project.",

year = "2002",

month = jan,

doi = "10.1016/S0927-6505(01)00110-4",

language = "אנגלית",

volume = "16",

pages = "205--234",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier B.V.",

number = "3",

}

Alimonti, G, Arpesella, C, Back, H, Balata, M, Beau, T, Bellini, G, Benziger, J, Bonetti, S, Brigatti, A, Caccianiga, B, Cadonati, L, Calaprice, F, Cecchet, G, Chen, M, DeBari, A, DeHaas, E, De Kerret, H, Donghi, O, Deutsch, M, Elisei, F, Etenko, A, Von Feilitzsch, F, Fernholz, R, Ford, R, Freudiger, B, Garagiola, A, Galbiati, C, Gatti, F, Gazzana, S, Giammarchi, M, Giugni, D, Golubchikov, A, Goretti, A, Grieb, C, Hagner, C, Hagner, T, Hampel, W, Harding, E, Hartmann, F, Von Hentig, R, Hess, H, Heusser, G, Ianni, A, Inzani, P, Kidner, S, Kiko, J, Kirsten, T, Korga, G, Korschinek, G, Kryn, D, Lagomarsino, V, LaMarcne, P, Laubenstein, M, Loeser, F, Lombardi, P, Magni, S, Malvezzi, S, Maniera, J, Manno, I, Manuzio, G, Masetti, F, Mazzucato, U, Meroni, E, Musico, P, Neder, H, Neff, M, Nisi, S, Oberauer, L, Obolensky, M, Pallavicini, M, Papp, L, Perasso, L, Pocar, A, Raghavan, R, Ranucci, G, Rau, W, Razeto, A, Resconi, E, Riedel, T, Sabelnikov, A, Saggese, P, Salvo, C, Scardaoni, R, Schoenert, S, Schuhbeck, K, Seidel, H, Shutt, T, Simgen, H, Sonnenschein, A, Smirnov, O, Sotnikov, A, Skorokhvatov, M, Sukhotin, S, Tartaglia, R, Testera, G, Vogelaar, R, Vitale, S, Wojcik, M, Zaimidoroga, O & Zakharov, Y 2002, 'Science and technology of Borexino: A real-time detector for low energy solar neutrinos', Astroparticle Physics, vol. 16, no. 3, pp. 205-234. https://doi.org/10.1016/S0927-6505(01)00110-4

TY - JOUR

T1 - Science and technology of Borexino

T2 - A real-time detector for low energy solar neutrinos

AU - Alimonti, G.

AU - Arpesella, C.

AU - Back, H.

AU - Balata, M.

AU - Beau, T.

AU - Bellini, G.

AU - Benziger, J.

AU - Bonetti, S.

AU - Brigatti, A.

AU - Caccianiga, B.

AU - Cadonati, L.

AU - Calaprice, F.

AU - Cecchet, G.

AU - Chen, M.

AU - DeBari, A.

AU - DeHaas, E.

AU - De Kerret, H.

AU - Donghi, O.

AU - Deutsch, M.

AU - Elisei, F.

AU - Etenko, A.

AU - Von Feilitzsch, F.

AU - Fernholz, R.

AU - Ford, R.

AU - Freudiger, B.

AU - Garagiola, A.

AU - Galbiati, C.

AU - Gatti, F.

AU - Gazzana, S.

AU - Giammarchi, M.

AU - Giugni, D.

AU - Golubchikov, A.

AU - Goretti, A.

AU - Grieb, C.

AU - Hagner, C.

AU - Hagner, T.

AU - Hampel, W.

AU - Harding, E.

AU - Hartmann, F.

AU - Von Hentig, R.

AU - Hess, H.

AU - Heusser, G.

AU - Ianni, A.

AU - Inzani, P.

AU - Kidner, S.

AU - Kiko, J.

AU - Kirsten, T.

AU - Korga, G.

AU - Korschinek, G.

AU - Kryn, D.

AU - Lagomarsino, V.

AU - LaMarcne, P.

AU - Laubenstein, M.

AU - Loeser, F.

AU - Lombardi, P.

AU - Magni, S.

AU - Malvezzi, S.

AU - Maniera, J.

AU - Manno, I.

AU - Manuzio, G.

AU - Masetti, F.

AU - Mazzucato, U.

AU - Meroni, E.

AU - Musico, P.

AU - Neder, H.

AU - Neff, M.

AU - Nisi, S.

AU - Oberauer, L.

AU - Obolensky, M.

AU - Pallavicini, M.

AU - Papp, L.

AU - Perasso, L.

AU - Pocar, A.

AU - Raghavan, R.

AU - Ranucci, G.

AU - Rau, W.

AU - Razeto, A.

AU - Resconi, E.

AU - Riedel, T.

AU - Sabelnikov, A.

AU - Saggese, P.

AU - Salvo, C.

AU - Scardaoni, R.

AU - Schoenert, S.

AU - Schuhbeck, K.

AU - Seidel, H.

AU - Shutt, T.

AU - Simgen, H.

AU - Sonnenschein, A.

AU - Smirnov, O.

AU - Sotnikov, A.

AU - Skorokhvatov, M.

AU - Sukhotin, S.

AU - Tartaglia, R.

AU - Testera, G.

AU - Vogelaar, R.

AU - Vitale, S.

AU - Wojcik, M.

AU - Zaimidoroga, O.

AU - Zakharov, Y.

N1 - Funding Information: Many individuals besides the authors have contributed to the development of the Borexino project. We wish to acknowledge particularly the following who made significant contributions in early stages: R. Cereseto, N. Darnton, A. Falgiani, T. Goldbrunner, J. Jochum, M. Johnson, A. Manco, A. Nostro, S. Pakvasa, M. Parodi, A. Perotti, G. Pieri, A. Preda, P. Raghavan, P. Rothschild, P. Ullucci and members of IRMM for the measurements made in Geel. The collaboration wants to thank the Laboratori Nazionali del Gran Sasso [LNGS] and A. Bettini for continuous help and support. We sincerely thank the funding bodies: Istituto Nazionale di Fisica Nucleare [INFN], and Ministero della Universita' e della Ricerca Scientifica e Tecnologica [MURST] (Italy); IN2P3 (France); Bundesministerium für Bildung, Wissenschaft, Forschung und Technologie [BMBF], Deutsche Forschungsgemeinschaft [DFG] and Max-Planck-Gesellschaft [MPG] (Germany); the National Science Foundation and Bell Laboratories (USA); the Natural Sciences and Engineering Research Council of Canada, and agencies in Hungary, Poland and Russia for their generous support of this project.

PY - 2002/1

Y1 - 2002/1

N2 - Borexino, a real-time device for low energy neutrino spectroscopy is nearing completion of construction in the underground laboratories at Gran Sasso, Italy (LNGS). The experiment's goal is the direct measurement of the flux of 7Be solar neutrinos of all flavors via neutrino-electron scattering in an ultra-pure scintillation liquid. Seeded by a series of innovations which were brought to fruition by large-scale operation of a 4-ton test detector at LNGS, a new technology has been developed for Borexino. It enables sub-MeV solar neutrino spectroscopy for the first time. This paper describes the design of Borexino, the various facilities essential to its operation, its spectroscopic and background suppression capabilities and a prognosis of the impact of its results towards resolving the solar neutrino problem. Borexino will also address several other frontier questions in particle physics, astrophysics and geophysics.

AB - Borexino, a real-time device for low energy neutrino spectroscopy is nearing completion of construction in the underground laboratories at Gran Sasso, Italy (LNGS). The experiment's goal is the direct measurement of the flux of 7Be solar neutrinos of all flavors via neutrino-electron scattering in an ultra-pure scintillation liquid. Seeded by a series of innovations which were brought to fruition by large-scale operation of a 4-ton test detector at LNGS, a new technology has been developed for Borexino. It enables sub-MeV solar neutrino spectroscopy for the first time. This paper describes the design of Borexino, the various facilities essential to its operation, its spectroscopic and background suppression capabilities and a prognosis of the impact of its results towards resolving the solar neutrino problem. Borexino will also address several other frontier questions in particle physics, astrophysics and geophysics.

UR - https://www.scopus.com/pages/publications/0013147397

U2 - 10.1016/S0927-6505(01)00110-4

DO - 10.1016/S0927-6505(01)00110-4

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???

AN - SCOPUS:0013147397

SN - 0927-6505

VL - 16

SP - 205

EP - 234

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 3

ER -

Science and technology of Borexino: A real-time detector for low energy solar neutrinos

Abstract

Bibliographical note

Funding

Access to Document

Other files and links

Fingerprint

Cite this