Search for 5.5 MeV solar axions produced in a, p(d,3He)A reaction with Borexino detector

A. Derbin; V. Muratova; 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; D. D'Angelo; S. Davini; A. Etenko; K. Fomenko; D. Franco; C. Galbiati; S. Gazzana; C. Ghiano; M. Giammarchi; M. Goeger-Neff; A. Goretti; L. Grandi; E. Guardincerri; S. Hardy; Al Ianni; An Ianni; A. Kayunov; V. Kobychev; D. Korablev; G. Korga; Y. Koshio; D. Kryn; M. Laubenstein; T. Lewke; E. Litvinovich; B. 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; L. Oberauer; M. Obolensky; F. Ortica; K. Otis; M. Pallavicini; L. Papp; L. Perasso; S. Perasso; A. Pocar; S. Raghavan; G. Ranucci; A. Razeto; A. Re; A. Romani; 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; F. Von Feilitzsch; J. Winter; M. Wojcik; A. Wright; M. Wurm; J. Xu; O. Zaimidoroga; S. Zavatarelli; G. Zuzel

doi:10.3204/DESY-PROC-2011-04/derbin_alexander

Search for 5.5 MeV solar axions produced in a, p(d,³He)A reaction with Borexino detector

A. Derbin, V. Muratova, 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, D. D'Angelo, S. Davini, A. Etenko, K. Fomenko, D. Franco, C. GalbiatiS. Gazzana, C. Ghiano, M. Giammarchi, M. Goeger-Neff, A. Goretti, L. Grandi, E. Guardincerri, S. Hardy, Al Ianni, An Ianni, A. Kayunov, V. Kobychev, D. Korablev, G. Korga, Y. Koshio, D. Kryn, M. Laubenstein, T. Lewke, E. Litvinovich, B. 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, L. Oberauer, M. Obolensky, F. Ortica, K. Otis, M. Pallavicini, L. Papp, L. Perasso, S. Perasso, A. Pocar, S. Raghavan, G. Ranucci, A. Razeto, A. Re, A. Romani, 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, F. Von Feilitzsch, J. Winter, M. Wojcik, A. Wright, M. Wurm, J. Xu, O. Zaimidoroga, S. Zavatarelli, G. Zuzel

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

A search for 5.5-MeV solar axions produced in the p + d →³He + Υ(5.5MeV) reaction, was performed using the Borexino detector. Model independent limits on axion-electron, (gAe), axion-photon (gAΥ), and isovector axion-nucleon (g3AN) couplings are obtained:, |gAe × g3AN| ≤ 5.5 × 10^-13and |gAΥ × g3AN| ≤ 4.6 × 10^-11GeV^-1at mA < 1 MeV (90%, c.l.). These limits are 2-4 orders of magnitude stronger than those obtained in previous, laboratory-based experiments using nuclear reactors and accelerators.

Original language	English
Title of host publication	Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011
Publisher	Verlag Deutsches Elektronen-Synchrotron
Pages	107-111
Number of pages	5
ISBN (Print)	9783935702591
DOIs	https://doi.org/10.3204/DESY-PROC-2011-04/derbin_alexander
Publication status	Published - 2011
Externally published	Yes
Event	7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011 - Mykonos, Greece Duration: Jun 27 2011 → Jul 1 2011

Publication series

Name	Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011

Other

Other	7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011
Country/Territory	Greece
City	Mykonos
Period	6/27/11 → 7/1/11

ASJC Scopus subject areas

Nuclear and High Energy Physics
Atomic and Molecular Physics, and Optics

Access to Document

10.3204/DESY-PROC-2011-04/derbin_alexander

Cite this

Derbin, A., Muratova, V., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Buizza Avanzini, M., Caccianiga, B., Cadonati, L., Calaprice, F., Carraro, C., Cavalcante, P., Chavarria, A., D'Angelo, D., Davini, S., Etenko, A., Fomenko, K., Franco, D., ... Zuzel, G. (2011). Search for 5.5 MeV solar axions produced in a, p(d,³He)A reaction with Borexino detector. In Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011 (pp. 107-111). (Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011). Verlag Deutsches Elektronen-Synchrotron. https://doi.org/10.3204/DESY-PROC-2011-04/derbin_alexander

Search for 5.5 MeV solar axions produced in a, p(d,³He)A reaction with Borexino detector. / Derbin, A.; Muratova, V.; Bellini, G. et al.
Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011. Verlag Deutsches Elektronen-Synchrotron, 2011. p. 107-111 (Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Derbin, A, Muratova, V, Bellini, G, Benziger, J, Bick, D, Bonfini, G, Bravo, D, Buizza Avanzini, M, Caccianiga, B, Cadonati, L, Calaprice, F, Carraro, C, Cavalcante, P, Chavarria, A, D'Angelo, D, Davini, S, Etenko, A, Fomenko, K, Franco, D, Galbiati, C, Gazzana, S, Ghiano, C, Giammarchi, M, Goeger-Neff, M, Goretti, A, Grandi, L, Guardincerri, E, Hardy, S, Ianni, A, Ianni, A, Kayunov, A, Kobychev, V, Korablev, D, Korga, G, Koshio, Y, Kryn, D, Laubenstein, M, Lewke, T, Litvinovich, E, Loer, B, Lombardi, F, Lombardi, P, Ludhova, L, Machulin, I, Manecki, S, Maneschg, W, Manuzio, G, Meindl, Q, Meroni, E, Miramonti, L, Misiaszek, M, Montanari, D, Mosteiro, P, Oberauer, L, Obolensky, M, Ortica, F, Otis, K, Pallavicini, M, Papp, L, Perasso, L, Perasso, S, Pocar, A, Raghavan, S, Ranucci, G, Razeto, A, Re, A, Romani, A, Sabelnikov, A, Saldanha, R, Salvo, C, Schönert, S, Simgen, H, Skorokhvatov, M, Smirnov, O, Sotnikov, A, Sukhotin, S, Suvorov, Y, Tartaglia, R, Testera, G, Vignaud, D, Vogelaar, RB, Von Feilitzsch, F, Winter, J, Wojcik, M, Wright, A, Wurm, M, Xu, J, Zaimidoroga, O, Zavatarelli, S & Zuzel, G 2011, Search for 5.5 MeV solar axions produced in a, p(d,³He)A reaction with Borexino detector. in Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011. Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011, Verlag Deutsches Elektronen-Synchrotron, pp. 107-111, 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011, Mykonos, Greece, 6/27/11. https://doi.org/10.3204/DESY-PROC-2011-04/derbin_alexander

Derbin A, Muratova V, Bellini G, Benziger J, Bick D, Bonfini G et al. Search for 5.5 MeV solar axions produced in a, p(d,³He)A reaction with Borexino detector. In Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011. Verlag Deutsches Elektronen-Synchrotron. 2011. p. 107-111. (Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011). doi: 10.3204/DESY-PROC-2011-04/derbin_alexander

@inproceedings{a86644b8c7ed44b795994b5455be4bf9,

title = "Search for 5.5 MeV solar axions produced in a, p(d,3He)A reaction with Borexino detector",

abstract = "A search for 5.5-MeV solar axions produced in the p + d →3He + Υ(5.5MeV) reaction, was performed using the Borexino detector. Model independent limits on axion-electron, (gAe), axion-photon (gAΥ), and isovector axion-nucleon (g3AN) couplings are obtained:, |gAe × g3AN| ≤ 5.5 × 10-13and |gAΥ × g3AN| ≤ 4.6 × 10-11GeV-1at mA < 1 MeV (90%, c.l.). These limits are 2-4 orders of magnitude stronger than those obtained in previous, laboratory-based experiments using nuclear reactors and accelerators.",

author = "A. Derbin and V. Muratova and G. Bellini and J. Benziger and D. Bick and G. Bonfini and D. Bravo and {Buizza Avanzini}, M. and B. Caccianiga and L. Cadonati and F. Calaprice and C. Carraro and P. Cavalcante and A. Chavarria and D. D'Angelo and S. Davini and A. Etenko and K. Fomenko and D. Franco and C. Galbiati and S. Gazzana and C. Ghiano and M. Giammarchi and M. Goeger-Neff and A. Goretti and L. Grandi and E. Guardincerri and S. Hardy and Al Ianni and An Ianni and A. Kayunov and V. Kobychev and D. Korablev and G. Korga and Y. Koshio and D. Kryn and M. Laubenstein and T. Lewke and E. Litvinovich and B. Loer and F. Lombardi and P. Lombardi and L. Ludhova and I. Machulin and S. Manecki and W. Maneschg and G. Manuzio and Q. Meindl and E. Meroni and L. Miramonti and M. Misiaszek and D. Montanari and P. Mosteiro and L. Oberauer and M. Obolensky and F. Ortica and K. Otis and M. Pallavicini and L. Papp and L. Perasso and S. Perasso and A. Pocar and S. Raghavan and G. Ranucci and A. Razeto and A. Re and A. Romani and A. Sabelnikov and R. Saldanha and C. Salvo and S. Sch{\"o}nert 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 D. Vignaud and Vogelaar, {R. B.} and {Von Feilitzsch}, F. and J. Winter and M. Wojcik and A. Wright and M. Wurm and J. Xu and O. Zaimidoroga and S. Zavatarelli and G. Zuzel",

year = "2011",

doi = "10.3204/DESY-PROC-2011-04/derbin_alexander",

language = "English",

isbn = "9783935702591",

series = "Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011",

publisher = "Verlag Deutsches Elektronen-Synchrotron",

pages = "107--111",

booktitle = "Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011",

note = "7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011 ; Conference date: 27-06-2011 Through 01-07-2011",

}

TY - GEN

T1 - Search for 5.5 MeV solar axions produced in a, p(d,3He)A reaction with Borexino detector

AU - Derbin, A.

AU - Muratova, V.

AU - Bellini, G.

AU - Benziger, J.

AU - Bick, D.

AU - Bonfini, G.

AU - Bravo, D.

AU - Buizza Avanzini, M.

AU - Caccianiga, B.

AU - Cadonati, L.

AU - Calaprice, F.

AU - Carraro, C.

AU - Cavalcante, P.

AU - Chavarria, A.

AU - D'Angelo, D.

AU - Davini, S.

AU - Etenko, A.

AU - Fomenko, K.

AU - Franco, D.

AU - Galbiati, C.

AU - Gazzana, S.

AU - Ghiano, C.

AU - Giammarchi, M.

AU - Goeger-Neff, M.

AU - Goretti, A.

AU - Grandi, L.

AU - Guardincerri, E.

AU - Hardy, S.

AU - Ianni, Al

AU - Ianni, An

AU - Kayunov, A.

AU - Kobychev, V.

AU - Korablev, D.

AU - Korga, G.

AU - Koshio, Y.

AU - Kryn, D.

AU - Laubenstein, M.

AU - Lewke, T.

AU - Litvinovich, E.

AU - Loer, B.

AU - Lombardi, F.

AU - Lombardi, P.

AU - Ludhova, L.

AU - Machulin, I.

AU - Manecki, S.

AU - Maneschg, W.

AU - Manuzio, G.

AU - Meindl, Q.

AU - Meroni, E.

AU - Miramonti, L.

AU - Misiaszek, M.

AU - Montanari, D.

AU - Mosteiro, P.

AU - Oberauer, L.

AU - Obolensky, M.

AU - Ortica, F.

AU - Otis, K.

AU - Pallavicini, M.

AU - Papp, L.

AU - Perasso, L.

AU - Perasso, S.

AU - Pocar, A.

AU - Raghavan, S.

AU - Ranucci, G.

AU - Razeto, A.

AU - Re, A.

AU - Romani, A.

AU - Sabelnikov, A.

AU - Saldanha, R.

AU - Salvo, C.

AU - Schönert, S.

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 - Vignaud, D.

AU - Vogelaar, R. B.

AU - Von Feilitzsch, F.

AU - Winter, J.

AU - Wojcik, M.

AU - Wright, A.

AU - Wurm, M.

AU - Xu, J.

AU - Zaimidoroga, O.

AU - Zavatarelli, S.

AU - Zuzel, G.

PY - 2011

Y1 - 2011

N2 - A search for 5.5-MeV solar axions produced in the p + d →3He + Υ(5.5MeV) reaction, was performed using the Borexino detector. Model independent limits on axion-electron, (gAe), axion-photon (gAΥ), and isovector axion-nucleon (g3AN) couplings are obtained:, |gAe × g3AN| ≤ 5.5 × 10-13and |gAΥ × g3AN| ≤ 4.6 × 10-11GeV-1at mA < 1 MeV (90%, c.l.). These limits are 2-4 orders of magnitude stronger than those obtained in previous, laboratory-based experiments using nuclear reactors and accelerators.

AB - A search for 5.5-MeV solar axions produced in the p + d →3He + Υ(5.5MeV) reaction, was performed using the Borexino detector. Model independent limits on axion-electron, (gAe), axion-photon (gAΥ), and isovector axion-nucleon (g3AN) couplings are obtained:, |gAe × g3AN| ≤ 5.5 × 10-13and |gAΥ × g3AN| ≤ 4.6 × 10-11GeV-1at mA < 1 MeV (90%, c.l.). These limits are 2-4 orders of magnitude stronger than those obtained in previous, laboratory-based experiments using nuclear reactors and accelerators.

UR - http://www.scopus.com/inward/record.url?scp=84880455328&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84880455328&partnerID=8YFLogxK

U2 - 10.3204/DESY-PROC-2011-04/derbin_alexander

DO - 10.3204/DESY-PROC-2011-04/derbin_alexander

M3 - Conference contribution

AN - SCOPUS:84880455328

SN - 9783935702591

T3 - Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011

SP - 107

EP - 111

BT - Proceedings of the 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011

PB - Verlag Deutsches Elektronen-Synchrotron

T2 - 7th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2011

Y2 - 27 June 2011 through 1 July 2011

ER -