Recent Results from Borexino

D. Jeschke; M. Agostini; K. Altenmüller; S. Appel; V. Atroshchenko; G. Bellini; J. Benziger; D. Bick; G. Bonfini; D. Bravo; B. Caccianiga; F. Calaprice; A. Caminata; M. Carlini; P. Cavalcante; A. Chepurnov; K. Choi; D. D'Angelo; S. Davini; A. Derbin; L. Di Noto; I. Drachnev; A. Etenko; K. Fomenko; D. Franco; F. Gabriele; C. Galbiati; C. Ghiano; M. Giammarchi; M. Goeger-Neff; A. Goretti; M. Gromov; C. Hagner; E. Hungerford; Aldo Ianni; Andrea Ianni; A. Jany; K. Jedrzejczak; D. Jeschke; V. Kobychev; D. Korablev; G. Korga; D. Kryn; M. Laubenstein; B. Lehnert; E. Litvinovich; F. Lombardi; P. Lombardi; L. Ludhova; G. Lukyanchenko; I. Machulin; S. Manecki; W. Maneschg; G. Manuzio; S. Marcocci; E. Meroni; M. Meyer; L. Miramonti; M. Misiaszek; M. Montuschi; P. Mosteiro; V. Muratova; B. Neumair; L. Oberauer; M. Obolensky; F. Ortica; M. Pallavicini; L. Papp; A. Pocar; G. Ranucci; A. Razeto; A. Re; A. Romani; R. Roncin; N. Rossi; S. Schönert; D. Semenov; M. Skorokhvatov; O. Smirnov; A. Sotnikov; S. Sukhotin; Y. Suvorov; R. Tartaglia; G. Testera; J. Thurn; M. Toropova; E. Unzhakov; A. Vishneva; R. B. Vogelaar; F. Von Feilitzsch; H. Wang; S. Weinz; J. Winter; M. Wojcik; M. Wurm; Z. Yokley; O. Zaimidoroga; S. Zavatarelli; K. Zuber; G. Zuzel

doi:10.1088/1742-6596/798/1/012114

Recent Results from Borexino

D. Jeschke
, M. Agostini
, K. Altenmüller
, S. Appel
, V. Atroshchenko
, G. Bellini
, J. Benziger
, D. Bick
, G. Bonfini
, D. Bravo
, B. Caccianiga
, F. Calaprice
, A. Caminata
, M. Carlini
, P. Cavalcante
, A. Chepurnov
, K. Choi
, D. D'Angelo
, S. Davini
, A. Derbin

L. Di Noto, I. Drachnev, A. Etenko, K. Fomenko, D. Franco, F. Gabriele, C. Galbiati, C. Ghiano, M. Giammarchi, M. Goeger-Neff, A. Goretti, M. Gromov, C. Hagner, E. Hungerford, Aldo Ianni, Andrea Ianni, A. Jany, K. Jedrzejczak, D. Jeschke, V. Kobychev, D. Korablev, G. Korga, D. Kryn, M. Laubenstein, B. Lehnert, E. Litvinovich, F. Lombardi, P. Lombardi, L. Ludhova, G. Lukyanchenko, I. Machulin, S. Manecki, W. Maneschg, G. Manuzio, S. Marcocci, E. Meroni, M. Meyer, L. Miramonti, M. Misiaszek, M. Montuschi, P. Mosteiro, V. Muratova, B. Neumair, L. Oberauer, M. Obolensky, F. Ortica, M. Pallavicini, L. Papp, A. Pocar, G. Ranucci, A. Razeto, A. Re, A. Romani, R. Roncin, N. Rossi, S. Schönert, D. Semenov, M. Skorokhvatov, O. Smirnov, A. Sotnikov, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, J. Thurn, M. Toropova, E. Unzhakov, A. Vishneva, R. B. Vogelaar, F. Von Feilitzsch, H. Wang, S. Weinz, J. Winter, M. Wojcik, M. Wurm, Z. Yokley, O. Zaimidoroga, S. Zavatarelli, K. Zuber, G. Zuzel

Cluster of Excellence E-conversion
Gran Sasso Science Institute
National Research Centre "Kurchatov Institute"
University of Milan
Department of Chemical Engineering
Universität Hamburg
Laboratori Nazionali del Gran Sasso
Virginia Polytechnic Institute and State University
Princeton University
Istituto Nazionale per la Fisica della Materia
Moscow State University
University of Hawaii
Petersburg Nuclear Phys. Inst.
Joint Inst. for Nuclear Research
Université Paris Diderot
Center for Nuclear Receptors and Cell Signaling, University of Houston
Jagiellonian University
Institute for Nuclear Research
Technische Universität Dresden
National Research Nuclear University MEPhI
RWTH Aachen University
Forschungszentrum Jülich (FZJ)
Queen's University
Max-Planck-Institut für Kernphysik
University of Ferrara
INFN Sezione di Perugia
University of Massachusetts Amherst
University of California at Los Angeles
Johannes Gutenberg University

Research output: Contribution to journal › Conference article › peer-review

1 Scopus citations

Abstract

The Borexino experiment is taking data since 2007 at the Laboratori Nazionali del Gran Sasso in Italy accomplishing outstanding achievements in the field of neutrino physics. Its success is strongly based on the unprecedented ultra-high radio-purity of the inner scintillator core. The main features of the detector and the impressive results for solar and geo-neutrinos obtained by Borexino so far are summarized. The main focus is laid on the most recent results, i.e. the first real-time measurement of the solar pp neutrino flux and the detection of the signal induced by geo-neutrinos with a significance as high as 5.9σ. The measurement of the pp neutrino flux represents a direct probe of the major mechanism of energy production in the Sun and its observation at a significance of 10σ proves the stability of the Sun over a time of at least 10⁵ years. It further puts Borexino in the unique position of being capable to test the MSW-LMA paradigm across the whole solar energy range. The geo-neutrino data allow to infer information concerning important geophysical properties of the Earth that are also discussed. The perspectives of the final stage of the Borexino solar neutrino program that are centered on the goal of measuring the CNO neutrinos that so far escaped any observation are outlined.

Original language	English
Article number	012114
Journal	Journal of Physics: Conference Series
Volume	798
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/798/1/012114
State	Published - 7 Mar 2017
Externally published	Yes
Event	2nd International Conference on Particle Physics and Astrophysics, ICPPA 2016 - Moscow, Russian Federation Duration: 10 Oct 2016 → 14 Oct 2016

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10.1088/1742-6596/798/1/012114

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Jeschke, D., Agostini, M., Altenmüller, K., Appel, S., Atroshchenko, V., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Carlini, M., Cavalcante, P., Chepurnov, A., Choi, K., D'Angelo, D., Davini, S., ... Zuzel, G. (2017). Recent Results from Borexino. Journal of Physics: Conference Series, 798(1), Article 012114. https://doi.org/10.1088/1742-6596/798/1/012114

@article{12e0845479284c6181555a41a1bcbe0a,

title = "Recent Results from Borexino",

abstract = "The Borexino experiment is taking data since 2007 at the Laboratori Nazionali del Gran Sasso in Italy accomplishing outstanding achievements in the field of neutrino physics. Its success is strongly based on the unprecedented ultra-high radio-purity of the inner scintillator core. The main features of the detector and the impressive results for solar and geo-neutrinos obtained by Borexino so far are summarized. The main focus is laid on the most recent results, i.e. the first real-time measurement of the solar pp neutrino flux and the detection of the signal induced by geo-neutrinos with a significance as high as 5.9σ. The measurement of the pp neutrino flux represents a direct probe of the major mechanism of energy production in the Sun and its observation at a significance of 10σ proves the stability of the Sun over a time of at least 105 years. It further puts Borexino in the unique position of being capable to test the MSW-LMA paradigm across the whole solar energy range. The geo-neutrino data allow to infer information concerning important geophysical properties of the Earth that are also discussed. The perspectives of the final stage of the Borexino solar neutrino program that are centered on the goal of measuring the CNO neutrinos that so far escaped any observation are outlined.",

author = "D. Jeschke and M. Agostini and K. Altenm{\"u}ller and S. Appel and V. Atroshchenko and G. Bellini and J. Benziger and D. Bick and G. Bonfini and D. Bravo and B. Caccianiga and F. Calaprice and A. Caminata and M. Carlini and P. Cavalcante and A. Chepurnov and K. Choi and D. D'Angelo and S. Davini and A. Derbin and \{Di Noto\}, L. and I. Drachnev and A. Etenko and K. Fomenko and D. Franco and F. Gabriele and C. Galbiati and C. Ghiano and M. Giammarchi and M. Goeger-Neff and A. Goretti and M. Gromov and C. Hagner and E. Hungerford and Aldo Ianni and Andrea Ianni and A. Jany and K. Jedrzejczak and D. Jeschke and V. Kobychev and D. Korablev and G. Korga and D. Kryn and M. Laubenstein and B. Lehnert and E. Litvinovich and F. Lombardi and P. Lombardi and L. Ludhova and G. Lukyanchenko and I. Machulin and S. Manecki and W. Maneschg and G. Manuzio and S. Marcocci and E. Meroni and M. Meyer and L. Miramonti and M. Misiaszek and M. Montuschi and P. Mosteiro and V. Muratova and B. Neumair and L. Oberauer and M. Obolensky and F. Ortica and M. Pallavicini and L. Papp and A. Pocar and G. Ranucci and A. Razeto and A. Re and A. Romani and R. Roncin and N. Rossi and S. Sch{\"o}nert and D. Semenov and M. Skorokhvatov and O. Smirnov and A. Sotnikov and S. Sukhotin and Y. Suvorov and R. Tartaglia and G. Testera and J. Thurn and M. Toropova and E. Unzhakov and A. Vishneva and Vogelaar, \{R. B.\} and \{Von Feilitzsch\}, F. and H. Wang and S. Weinz and J. Winter and M. Wojcik and M. Wurm and Z. Yokley and O. Zaimidoroga and S. Zavatarelli and K. Zuber and G. Zuzel",

note = "Publisher Copyright: {\textcopyright} Published under licence by IOP Publishing Ltd.; 2nd International Conference on Particle Physics and Astrophysics, ICPPA 2016 ; Conference date: 10-10-2016 Through 14-10-2016",

year = "2017",

month = mar,

day = "7",

doi = "10.1088/1742-6596/798/1/012114",

language = "English",

volume = "798",

journal = "Journal of Physics: Conference Series",

issn = "1742-6588",

publisher = "IOP Publishing Ltd.",

number = "1",

}

Jeschke, D, Agostini, M, Altenmüller, K, Appel, S, Atroshchenko, V, Bellini, G, Benziger, J, Bick, D, Bonfini, G, Bravo, D, Caccianiga, B, Calaprice, F, Caminata, A, Carlini, M, Cavalcante, P, Chepurnov, A, Choi, K, D'Angelo, D, Davini, S, Derbin, A, Di Noto, L, Drachnev, I, Etenko, A, Fomenko, K, Franco, D, Gabriele, F, Galbiati, C, Ghiano, C, Giammarchi, M, Goeger-Neff, M, Goretti, A, Gromov, M, Hagner, C, Hungerford, E, Ianni, A, Ianni, A, Jany, A, Jedrzejczak, K, Jeschke, D, Kobychev, V, Korablev, D, Korga, G, Kryn, D, Laubenstein, M, Lehnert, B, Litvinovich, E, Lombardi, F, Lombardi, P, Ludhova, L, Lukyanchenko, G, Machulin, I, Manecki, S, Maneschg, W, Manuzio, G, Marcocci, S, Meroni, E, Meyer, M, Miramonti, L, Misiaszek, M, Montuschi, M, Mosteiro, P, Muratova, V, Neumair, B, Oberauer, L, Obolensky, M, Ortica, F, Pallavicini, M, Papp, L, Pocar, A, Ranucci, G, Razeto, A, Re, A, Romani, A, Roncin, R, Rossi, N, Schönert, S, Semenov, D, Skorokhvatov, M, Smirnov, O, Sotnikov, A, Sukhotin, S, Suvorov, Y, Tartaglia, R, Testera, G, Thurn, J, Toropova, M, Unzhakov, E, Vishneva, A, Vogelaar, RB, Von Feilitzsch, F, Wang, H, Weinz, S, Winter, J, Wojcik, M, Wurm, M, Yokley, Z, Zaimidoroga, O, Zavatarelli, S, Zuber, K & Zuzel, G 2017, 'Recent Results from Borexino', Journal of Physics: Conference Series, vol. 798, no. 1, 012114. https://doi.org/10.1088/1742-6596/798/1/012114

TY - JOUR

T1 - Recent Results from Borexino

AU - Jeschke, D.

AU - Agostini, M.

AU - Altenmüller, K.

AU - Appel, S.

AU - Atroshchenko, V.

AU - Bellini, G.

AU - Benziger, J.

AU - Bick, D.

AU - Bonfini, G.

AU - Bravo, D.

AU - Caccianiga, B.

AU - Calaprice, F.

AU - Caminata, A.

AU - Carlini, M.

AU - Cavalcante, P.

AU - Chepurnov, A.

AU - Choi, K.

AU - D'Angelo, D.

AU - Davini, S.

AU - Derbin, A.

AU - Di Noto, L.

AU - Drachnev, I.

AU - Etenko, A.

AU - Fomenko, K.

AU - Franco, D.

AU - Gabriele, F.

AU - Galbiati, C.

AU - Ghiano, C.

AU - Giammarchi, M.

AU - Goeger-Neff, M.

AU - Goretti, A.

AU - Gromov, M.

AU - Hagner, C.

AU - Hungerford, E.

AU - Ianni, Aldo

AU - Ianni, Andrea

AU - Jany, A.

AU - Jedrzejczak, K.

AU - Jeschke, D.

AU - Kobychev, V.

AU - Korablev, D.

AU - Korga, G.

AU - Kryn, D.

AU - Laubenstein, M.

AU - Lehnert, B.

AU - Litvinovich, E.

AU - Lombardi, F.

AU - Lombardi, P.

AU - Ludhova, L.

AU - Lukyanchenko, G.

AU - Machulin, I.

AU - Manecki, S.

AU - Maneschg, W.

AU - Manuzio, G.

AU - Marcocci, S.

AU - Meroni, E.

AU - Meyer, M.

AU - Miramonti, L.

AU - Misiaszek, M.

AU - Montuschi, M.

AU - Mosteiro, P.

AU - Muratova, V.

AU - Neumair, B.

AU - Oberauer, L.

AU - Obolensky, M.

AU - Ortica, F.

AU - Pallavicini, M.

AU - Papp, L.

AU - Pocar, A.

AU - Ranucci, G.

AU - Razeto, A.

AU - Re, A.

AU - Romani, A.

AU - Roncin, R.

AU - Rossi, N.

AU - Schönert, S.

AU - Semenov, D.

AU - Skorokhvatov, M.

AU - Smirnov, O.

AU - Sotnikov, A.

AU - Sukhotin, S.

AU - Suvorov, Y.

AU - Tartaglia, R.

AU - Testera, G.

AU - Thurn, J.

AU - Toropova, M.

AU - Unzhakov, E.

AU - Vishneva, A.

AU - Vogelaar, R. B.

AU - Von Feilitzsch, F.

AU - Wang, H.

AU - Weinz, S.

AU - Winter, J.

AU - Wojcik, M.

AU - Wurm, M.

AU - Yokley, Z.

AU - Zaimidoroga, O.

AU - Zavatarelli, S.

AU - Zuber, K.

AU - Zuzel, G.

PY - 2017/3/7

Y1 - 2017/3/7

N2 - The Borexino experiment is taking data since 2007 at the Laboratori Nazionali del Gran Sasso in Italy accomplishing outstanding achievements in the field of neutrino physics. Its success is strongly based on the unprecedented ultra-high radio-purity of the inner scintillator core. The main features of the detector and the impressive results for solar and geo-neutrinos obtained by Borexino so far are summarized. The main focus is laid on the most recent results, i.e. the first real-time measurement of the solar pp neutrino flux and the detection of the signal induced by geo-neutrinos with a significance as high as 5.9σ. The measurement of the pp neutrino flux represents a direct probe of the major mechanism of energy production in the Sun and its observation at a significance of 10σ proves the stability of the Sun over a time of at least 105 years. It further puts Borexino in the unique position of being capable to test the MSW-LMA paradigm across the whole solar energy range. The geo-neutrino data allow to infer information concerning important geophysical properties of the Earth that are also discussed. The perspectives of the final stage of the Borexino solar neutrino program that are centered on the goal of measuring the CNO neutrinos that so far escaped any observation are outlined.

AB - The Borexino experiment is taking data since 2007 at the Laboratori Nazionali del Gran Sasso in Italy accomplishing outstanding achievements in the field of neutrino physics. Its success is strongly based on the unprecedented ultra-high radio-purity of the inner scintillator core. The main features of the detector and the impressive results for solar and geo-neutrinos obtained by Borexino so far are summarized. The main focus is laid on the most recent results, i.e. the first real-time measurement of the solar pp neutrino flux and the detection of the signal induced by geo-neutrinos with a significance as high as 5.9σ. The measurement of the pp neutrino flux represents a direct probe of the major mechanism of energy production in the Sun and its observation at a significance of 10σ proves the stability of the Sun over a time of at least 105 years. It further puts Borexino in the unique position of being capable to test the MSW-LMA paradigm across the whole solar energy range. The geo-neutrino data allow to infer information concerning important geophysical properties of the Earth that are also discussed. The perspectives of the final stage of the Borexino solar neutrino program that are centered on the goal of measuring the CNO neutrinos that so far escaped any observation are outlined.

UR - https://www.scopus.com/pages/publications/85016253758

U2 - 10.1088/1742-6596/798/1/012114

DO - 10.1088/1742-6596/798/1/012114

M3 - Conference article

AN - SCOPUS:85016253758

SN - 1742-6588

VL - 798

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

IS - 1

M1 - 012114

T2 - 2nd International Conference on Particle Physics and Astrophysics, ICPPA 2016

Y2 - 10 October 2016 through 14 October 2016

ER -

Recent Results from Borexino

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