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Search for solar axions produced in the p(d, He-3)A reaction with Borexino detector

Author(s): Bellini, G; Benziger, Jay B.; Bick, D; Bonfini, G; Bravo, D; et al

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dc.contributor.authorBellini, G-
dc.contributor.authorBenziger, Jay B.-
dc.contributor.authorBick, D-
dc.contributor.authorBonfini, G-
dc.contributor.authorBravo, D-
dc.contributor.authorAvanzini, M Buizza-
dc.contributor.authorCaccianiga, B-
dc.contributor.authorCadonati, L-
dc.contributor.authorCalaprice, Frank P.-
dc.contributor.authorCarraro, C-
dc.contributor.authorCavalcante, P-
dc.contributor.authorChavarria, A-
dc.contributor.authorD Angelo, D-
dc.contributor.authorDavini, S-
dc.contributor.authorDerbin, A-
dc.contributor.authorEtenko, A-
dc.contributor.authorFomenko, K-
dc.contributor.authorFranco, D-
dc.contributor.authorGalbiati, Cristiano-
dc.contributor.authorGazzana, S-
dc.contributor.authorGhiano, C-
dc.contributor.authorGiammarchi, M-
dc.contributor.authorGoeger-Neff, M-
dc.contributor.authorGoretti, A-
dc.contributor.authorGrandi, L-
dc.contributor.authorGuardincerri, E-
dc.contributor.authorHardy, S-
dc.contributor.authorIanni, Aldo-
dc.contributor.authorIanni, Andrea-
dc.contributor.authorKayunov, A-
dc.contributor.authorKobychev, A-
dc.contributor.authorKorablev, D-
dc.contributor.authorKorga, G-
dc.contributor.authorKoshio, Y-
dc.contributor.authorKryn, D-
dc.contributor.authorLaubenstein, M-
dc.contributor.authorLewke, L-
dc.contributor.authorLitvinovich, E-
dc.contributor.authorLoer, B-
dc.contributor.authorLombardi, F-
dc.contributor.authorLombardi, P-
dc.contributor.authorLudhova, L-
dc.contributor.authorMachulin, I-
dc.contributor.authorManecki, S-
dc.contributor.authorManeschg, W-
dc.contributor.authorManuzio, G-
dc.contributor.authorMeindl, Q-
dc.contributor.authorMeroni, E-
dc.contributor.authorMiramonti, L-
dc.contributor.authorMisiaszek, M-
dc.contributor.authorMontanari, D-
dc.contributor.authorMosteiro, P-
dc.contributor.authorMuratova, V-
dc.contributor.authorOberauer, L-
dc.contributor.authorObolensky, M-
dc.contributor.authorOrtica, F-
dc.contributor.authorOtis, K-
dc.contributor.authorPallavicini, M-
dc.contributor.authorPapp, L-
dc.contributor.authorPerasso, L-
dc.contributor.authorPerasso, S-
dc.contributor.authorPocar, A-
dc.contributor.authorRaghavan, RS-
dc.contributor.authorRanucci, G-
dc.contributor.authorRazeto, A-
dc.contributor.authorRe, A-
dc.contributor.authorRomani, PA-
dc.contributor.authorSabelnikov, A-
dc.contributor.authorSaldanha, R-
dc.contributor.authorSalvo, C-
dc.contributor.authorSchoenert, S-
dc.contributor.authorSimgen, H-
dc.contributor.authorSkorokhvatov, M-
dc.contributor.authorSmirnov, O-
dc.contributor.authorSotnikov, A-
dc.contributor.authorSukhotin, S-
dc.contributor.authorSuvorov, Y-
dc.contributor.authorTartaglia, R-
dc.contributor.authorTestera, G-
dc.contributor.authorVignaud, D-
dc.contributor.authorVogelaar, RB-
dc.contributor.authorvon Feilitzsch, F-
dc.contributor.authorWinter, J-
dc.contributor.authorWojcik, M-
dc.contributor.authorWright, A-
dc.contributor.authorWurm, M-
dc.contributor.authorXu, J-
dc.contributor.authorZaimidoroga, O-
dc.contributor.authorZavatarelli, S-
dc.contributor.authorZuzel, G-
dc.contributor.authorCollaboration, Borexino-
dc.date.accessioned2019-08-29T17:06:06Z-
dc.date.available2019-08-29T17:06:06Z-
dc.date.issued2012-05-01en_US
dc.identifier.citationBellini, G, Benziger, J, Bick, D, Bonfini, G, Bravo, D, Avanzini, M Buizza, Caccianiga, B, Cadonati, L, Calaprice, F, Carraro, C, Cavalcante, P, Chavarria, A, D Angelo, D, Davini, S, Derbin, A, 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, Aldo, Ianni, Andrea, Kayunov, A, Kobychev, A, Korablev, D, Korga, G, Koshio, Y, Kryn, D, Laubenstein, M, Lewke, L, 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, Muratova, V, Oberauer, L, Obolensky, M, Ortica, F, Otis, K, Pallavicini, M, Papp, L, Perasso, L, Perasso, S, Pocar, A, Raghavan, RS, Ranucci, G, Razeto, A, Re, A, Romani, PA, Sabelnikov, A, Saldanha, R, Salvo, C, Schoenert, 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, Collaboration, Borexino. (2012). Search for solar axions produced in the p(d, He-3)A reaction with Borexino detector. PHYSICAL REVIEW D, 85 (10.1103/PhysRevD.85.092003en_US
dc.identifier.issn1550-7998-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1k14m-
dc.description.abstractA search for 5.5 MeV solar axions produced in the p + d -> He-3 + A (5.5 MeV) reaction was performed using the Borexino detector. The Compton conversion of axions to photons, A + e -> e + gamma; the axioelectric effect, A + e + Z -> e + Z; the decay of axions into two photons, A -> 2 gamma; and inverse Primakoff conversion on nuclei, A + Z -> gamma + Z, are considered. Model-independent limits on axion-electron (g(Ae)), axion-photon (g(A gamma)), and isovector axion-nucleon (g(3AN)) couplings are obtained: vertical bar g(Ae) x g(3AN)vertical bar <= 5.5 x 10(-13) and vertical bar g(A gamma) x g(3AN)vertical bar <= 4.6 x 10(-11) GeV-1 at m(A) < 1 MeV (90% confidence level). These limits are 2-4 orders of magnitude stronger than those obtained in previous laboratory-based experiments using nuclear reactors and accelerators.en_US
dc.language.isoen_USen_US
dc.relation.ispartofPHYSICAL REVIEW Den_US
dc.rightsAuthor's manuscripten_US
dc.titleSearch for solar axions produced in the p(d, He-3)A reaction with Borexino detectoren_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1103/PhysRevD.85.092003-
dc.date.eissued2012-05-04en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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