Radioactive source experiments in Borexino

Th Lasserre; K. Altenmueller; M. Agostini; S. Appel; G. Bellini; J. Benziger; N. Berton; D. Bick; G. Bonfini; D. Bravo; B. Caccianiga; F. Calaprice; A. Caminata; P. Cavalcante; A. Chepurnov; K. Choi; M. Cribier; D. D'Angelo; S. Davini; A. Derbin; L. Di Noto; I. Drachnev; M. Durero; A. Empl; A. Etenko; V. Fischer; G. Fiorentini; K. Fomenko; D. Franco; F. Gabriele; J. Gaffiot; C. Galbiati; C. Ghiano; M. Giammarchi; M. Goeger-Neff; A. Goretti; M. Gromov; C. Hagner; Th Houdy; E. Hungerford; A. Ianni; A. Ianni; K. Jedrzejczak; N. Jonqueres; M. Kaiser; V. Kobychev; D. Korablev; G. Korga; V. Kornoukhov; D. Kryn; M. Laubenstein; B. Lehnert; J. Link; E. Litvinovich; F. Lombardi; P. Lombardi; L. Ludhova; G. Lukyanchenko; I. Machulin; S. Manecki; W. Maneschg; F. Mantovani; S. Marcocci; E. Meroni; M. Meyer; L. Miramonti; M. Misiaszek; M. Montuschi; P. Mosteiro; V. Muratova; B. Neumair; L. Oberauer; M. Obolensky; F. Ortica; K. Otis; L. Pagani; M. Pallavicini; L. Papp; L. Perasso; A. Pocar; G. Ranucci; A. Razeto; B. Ricci; R. Roncin; N. Rossi; S. Schönert; D. Semenov; H. Simgen; M. Skorokhvatov; O. Smirnov; A. Sotnikov; S. Sukhotin; Y. Suvorov; R. Tartaglia; G. Testera; J. Thurn; M. Toropova; E. Unzhakov; C. Veyssiere; M. Vivier; 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

Radioactive source experiments in Borexino

Th Lasserre
, K. Altenmueller
, M. Agostini
, S. Appel
, G. Bellini
, J. Benziger
, N. Berton
, D. Bick
, G. Bonfini
, D. Bravo
, B. Caccianiga
, F. Calaprice
, A. Caminata
, P. Cavalcante
, A. Chepurnov
, K. Choi
, M. Cribier
, D. D'Angelo
, S. Davini
, A. Derbin

L. Di Noto, I. Drachnev, M. Durero, A. Empl, A. Etenko, V. Fischer, G. Fiorentini, K. Fomenko, D. Franco, F. Gabriele, J. Gaffiot, C. Galbiati, C. Ghiano, M. Giammarchi, M. Goeger-Neff, A. Goretti, M. Gromov, C. Hagner, Th Houdy, E. Hungerford, A. Ianni, A. Ianni, K. Jedrzejczak, N. Jonqueres, M. Kaiser, V. Kobychev, D. Korablev, G. Korga, V. Kornoukhov, D. Kryn, M. Laubenstein, B. Lehnert, J. Link, E. Litvinovich, F. Lombardi, P. Lombardi, L. Ludhova, G. Lukyanchenko, I. Machulin, S. Manecki, W. Maneschg, F. Mantovani, S. Marcocci, E. Meroni, M. Meyer, L. Miramonti, M. Misiaszek, M. Montuschi, P. Mosteiro, V. Muratova, B. Neumair, L. Oberauer, M. Obolensky, F. Ortica, K. Otis, L. Pagani, M. Pallavicini, L. Papp, L. Perasso, A. Pocar, G. Ranucci, A. Razeto, B. Ricci, R. Roncin, N. Rossi, S. Schönert, D. Semenov, H. Simgen, M. Skorokhvatov, O. Smirnov, A. Sotnikov, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, J. Thurn, M. Toropova, E. Unzhakov, C. Veyssiere, M. Vivier, 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

Commissariat A l'Énergie Atomique et Aux Énergies Alternatives, Centre de Saclay, IRFU
Université Paris Diderot
Cluster of Excellence E-conversion
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
Gran Sasso Science Institute
Petersburg Nuclear Phys. Inst.
Center for Nuclear Receptors and Cell Signaling, University of Houston
National Research Centre "Kurchatov Institute"
University of Ferrara
Joint Inst. for Nuclear Research
Jagiellonian University
Institute for Nuclear Research
ITEP
Technische Universität Dresden
Max-Planck-Institut für Kernphysik
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

Most of the neutrino oscillation results can be explained by the three-neutrino paradigm. However several anomalies in short baseline oscillation data (L/E of about 1 m/MeV) could be interpreted by invoking a light sterile neutrino. This new state would be separated from the standard neutrinos by a squared mass difference Δm²_new ∼ 0.1-1 eV² and would have mixing angles of sin² 2θ_ee ≳ 0.01 in the electron disappearance channel. This new neutrino, often called sterile, would not feel standard model interactions but mix with the others. We present the CeSOX and CrSOX projects to constrain the existence of eV-scale sterile neutrinos by deploying an intense radioactive β-source next to the Borexino detector.

Original language	English
Article number	025
Journal	Proceedings of Science
Volume	2-6-March-2015
State	Published - 2015
Externally published	Yes
Event	16th International Workshop on Neutrino Telescopes, NEUTEL 2015 - Venice, Italy Duration: 2 Mar 2015 → 6 Mar 2015

Cite this

Lasserre, T., Altenmueller, K., Agostini, M., Appel, S., Bellini, G., Benziger, J., Berton, N., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Cavalcante, P., Chepurnov, A., Choi, K., Cribier, M., D'Angelo, D., Davini, S., ... Zuzel, G. (2015). Radioactive source experiments in Borexino. Proceedings of Science, 2-6-March-2015, Article 025.

@article{df69b909cb5a4dab8740eb2e56f27ba5,

title = "Radioactive source experiments in Borexino",

abstract = "Most of the neutrino oscillation results can be explained by the three-neutrino paradigm. However several anomalies in short baseline oscillation data (L/E of about 1 m/MeV) could be interpreted by invoking a light sterile neutrino. This new state would be separated from the standard neutrinos by a squared mass difference Δm2new ∼ 0.1-1 eV2 and would have mixing angles of sin2 2θee ≳ 0.01 in the electron disappearance channel. This new neutrino, often called sterile, would not feel standard model interactions but mix with the others. We present the CeSOX and CrSOX projects to constrain the existence of eV-scale sterile neutrinos by deploying an intense radioactive β-source next to the Borexino detector.",

author = "Th Lasserre and K. Altenmueller and M. Agostini and S. Appel and G. Bellini and J. Benziger and N. Berton and D. Bick and G. Bonfini and D. Bravo and B. Caccianiga and F. Calaprice and A. Caminata and P. Cavalcante and A. Chepurnov and K. Choi and M. Cribier and D. D'Angelo and S. Davini and A. Derbin and \{Di Noto\}, L. and I. Drachnev and M. Durero and A. Empl and A. Etenko and V. Fischer and G. Fiorentini and K. Fomenko and D. Franco and F. Gabriele and J. Gaffiot and C. Galbiati and C. Ghiano and M. Giammarchi and M. Goeger-Neff and A. Goretti and M. Gromov and C. Hagner and Th Houdy and E. Hungerford and A. Ianni and A. Ianni and K. Jedrzejczak and N. Jonqueres and M. Kaiser and V. Kobychev and D. Korablev and G. Korga and V. Kornoukhov and D. Kryn and M. Laubenstein and B. Lehnert and J. Link 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 F. Mantovani 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 K. Otis and L. Pagani and M. Pallavicini and L. Papp and L. Perasso and A. Pocar and G. Ranucci and A. Razeto and B. Ricci and R. Roncin and N. Rossi and S. Sch{\"o}nert and D. Semenov and H. Simgen 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 C. Veyssiere and M. Vivier 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} Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.; 16th International Workshop on Neutrino Telescopes, NEUTEL 2015 ; Conference date: 02-03-2015 Through 06-03-2015",

year = "2015",

language = "English",

volume = "2-6-March-2015",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

Lasserre, T, Altenmueller, K, Agostini, M, Appel, S, Bellini, G, Benziger, J, Berton, N, Bick, D, Bonfini, G, Bravo, D, Caccianiga, B, Calaprice, F, Caminata, A, Cavalcante, P, Chepurnov, A, Choi, K, Cribier, M, D'Angelo, D, Davini, S, Derbin, A, Di Noto, L, Drachnev, I, Durero, M, Empl, A, Etenko, A, Fischer, V, Fiorentini, G, Fomenko, K, Franco, D, Gabriele, F, Gaffiot, J, Galbiati, C, Ghiano, C, Giammarchi, M, Goeger-Neff, M, Goretti, A, Gromov, M, Hagner, C, Houdy, T, Hungerford, E, Ianni, A, Ianni, A, Jedrzejczak, K, Jonqueres, N, Kaiser, M, Kobychev, V, Korablev, D, Korga, G, Kornoukhov, V, Kryn, D, Laubenstein, M, Lehnert, B, Link, J, Litvinovich, E, Lombardi, F, Lombardi, P, Ludhova, L, Lukyanchenko, G, Machulin, I, Manecki, S, Maneschg, W, Mantovani, F, Marcocci, S, Meroni, E, Meyer, M, Miramonti, L, Misiaszek, M, Montuschi, M, Mosteiro, P, Muratova, V, Neumair, B, Oberauer, L, Obolensky, M, Ortica, F, Otis, K, Pagani, L, Pallavicini, M, Papp, L, Perasso, L, Pocar, A, Ranucci, G, Razeto, A, Ricci, B, Roncin, R, Rossi, N, Schönert, S, Semenov, D, Simgen, H, Skorokhvatov, M, Smirnov, O, Sotnikov, A, Sukhotin, S, Suvorov, Y, Tartaglia, R, Testera, G, Thurn, J, Toropova, M, Unzhakov, E, Veyssiere, C, Vivier, M, 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 2015, 'Radioactive source experiments in Borexino', Proceedings of Science, vol. 2-6-March-2015, 025.

TY - JOUR

T1 - Radioactive source experiments in Borexino

AU - Lasserre, Th

AU - Altenmueller, K.

AU - Agostini, M.

AU - Appel, S.

AU - Bellini, G.

AU - Benziger, J.

AU - Berton, N.

AU - Bick, D.

AU - Bonfini, G.

AU - Bravo, D.

AU - Caccianiga, B.

AU - Calaprice, F.

AU - Caminata, A.

AU - Cavalcante, P.

AU - Chepurnov, A.

AU - Choi, K.

AU - Cribier, M.

AU - D'Angelo, D.

AU - Davini, S.

AU - Derbin, A.

AU - Di Noto, L.

AU - Drachnev, I.

AU - Durero, M.

AU - Empl, A.

AU - Etenko, A.

AU - Fischer, V.

AU - Fiorentini, G.

AU - Fomenko, K.

AU - Franco, D.

AU - Gabriele, F.

AU - Gaffiot, J.

AU - Galbiati, C.

AU - Ghiano, C.

AU - Giammarchi, M.

AU - Goeger-Neff, M.

AU - Goretti, A.

AU - Gromov, M.

AU - Hagner, C.

AU - Houdy, Th

AU - Hungerford, E.

AU - Ianni, A.

AU - Jedrzejczak, K.

AU - Jonqueres, N.

AU - Kaiser, M.

AU - Kobychev, V.

AU - Korablev, D.

AU - Korga, G.

AU - Kornoukhov, V.

AU - Kryn, D.

AU - Laubenstein, M.

AU - Lehnert, B.

AU - Link, J.

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 - Mantovani, F.

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 - Otis, K.

AU - Pagani, L.

AU - Pallavicini, M.

AU - Papp, L.

AU - Perasso, L.

AU - Pocar, A.

AU - Ranucci, G.

AU - Razeto, A.

AU - Ricci, B.

AU - Roncin, R.

AU - Rossi, N.

AU - Schönert, S.

AU - Semenov, D.

AU - Simgen, H.

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 - Veyssiere, C.

AU - Vivier, M.

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.

N1 - Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.

PY - 2015

Y1 - 2015

N2 - Most of the neutrino oscillation results can be explained by the three-neutrino paradigm. However several anomalies in short baseline oscillation data (L/E of about 1 m/MeV) could be interpreted by invoking a light sterile neutrino. This new state would be separated from the standard neutrinos by a squared mass difference Δm2new ∼ 0.1-1 eV2 and would have mixing angles of sin2 2θee ≳ 0.01 in the electron disappearance channel. This new neutrino, often called sterile, would not feel standard model interactions but mix with the others. We present the CeSOX and CrSOX projects to constrain the existence of eV-scale sterile neutrinos by deploying an intense radioactive β-source next to the Borexino detector.

AB - Most of the neutrino oscillation results can be explained by the three-neutrino paradigm. However several anomalies in short baseline oscillation data (L/E of about 1 m/MeV) could be interpreted by invoking a light sterile neutrino. This new state would be separated from the standard neutrinos by a squared mass difference Δm2new ∼ 0.1-1 eV2 and would have mixing angles of sin2 2θee ≳ 0.01 in the electron disappearance channel. This new neutrino, often called sterile, would not feel standard model interactions but mix with the others. We present the CeSOX and CrSOX projects to constrain the existence of eV-scale sterile neutrinos by deploying an intense radioactive β-source next to the Borexino detector.

UR - https://www.scopus.com/pages/publications/84988664664

M3 - Conference article

AN - SCOPUS:84988664664

SN - 1824-8039

VL - 2-6-March-2015

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 025

T2 - 16th International Workshop on Neutrino Telescopes, NEUTEL 2015

Y2 - 2 March 2015 through 6 March 2015

ER -

Radioactive source experiments in Borexino

Abstract

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