Searches for axioelectric effect of solar axions with BGO-scintillator and BGO-bolometer detectors

Muratova, V. N.; Gotti, C.; Bellini, F.; Maino, M.; Bakhlanov, S. V.; Capelli, S.; Maiano, C.; Kayunov, A. S.; Nagorny, S. S; Derbin, A. V.; Pirro, S.; Semenov, D. A.; Pavan, M.; Beeman, J. W.; Sisti, M.; Pattavina, L.; Giorni, L.; Ferri, E.; Dratchnev, I. S.; Biassoni, M.; Clemenza, M.; Giachero, A.; Unzhakov, E. V.

Contribution to a conference proceedings/Contribution to a book

PUBDB-2016-05923

Searches for axioelectric effect of solar axions with BGO-scintillator and BGO-bolometer detectors

Muratova, V. N. ; Derbin, A. V. ; Giorni, L. ; Nagorny, S. S. ; Pattavina, L. ; Bakhlanov, S. V. ; Beeman, J. W. ; Bellini, F. ; Biassoni, M. ; Capelli, S. ; Clemenza, M. ; Dratchnev, I. S. ; Ferri, E. ; Giachero, A. ; Gotti, C. ; Kayunov, A. S. ; Maiano, C. ; Maino, M. ; Pavan, M. ; Pirro, S. ; Semenov, D. A. ; Sisti, M. ; Unzhakov, E. V.

2014
Verlag Deutsches Elektronen-Synchrotron Hamburg
ISBN: 978-3-935702-59-1

Muratova, V.N. "Searches for axioelectric effect of solar axions with BGO-scintillator and BGO-bolometer detectors" in Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 : 10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29 - 2014-07-04, Geneva
10th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2014, Geneva, Switzerland, 29 Jun 2014 - 4 Jul 2014 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 117-120 (2014) [10.3204/DESY-PROC-2014-03/muratova_valentina]

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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2014-03/muratova_valentina

Abstract: A search for axioelectric absorption of 5.5 MeV solar axions produced in the $p + d \rightarrow {^3\rm{He}}+\gamma~(5.5~ \rm{MeV})$ reaction has been performed with a BGO detectors. A model-independent limit on the product of axion-nucleon $g_{AN}^3$ and axion-electron $g_{e}$ coupling constants has been obtained: $| g_{Ae}\times g_{AN}^3|< 1.9\times 10^{-10}$ for 90\% C.L..

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