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. DerbinL. 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

Publikation: Beitrag in Fachzeitschrift › Konferenzartikel › Begutachtung

1 Zitat (Scopus)

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.

Originalsprache	Englisch
Aufsatznummer	025
Fachzeitschrift	Proceedings of Science
Jahrgang	2-6-March-2015
Publikationsstatus	Veröffentlicht - 2015
Extern publiziert	Ja
Veranstaltung	16th International Workshop on Neutrino Telescopes, NEUTEL 2015 - Venice, Italien Dauer: 2 März 2015 → 6 März 2015

Andere Dateien und Links

Verknüpfung zur Publikation in Scopus

Dieses zitieren

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, Artikel 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, Jg. 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 - http://www.scopus.com/inward/record.url?scp=84988664664&partnerID=8YFLogxK

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

Andere Dateien und Links

Fingerprint

Dieses zitieren