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000315516 020__ $$a978-3-935702-59-1
000315516 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2014-03/muratova_valentina
000315516 0247_ $$2ISSN$$a1435-8077
000315516 037__ $$aPUBDB-2016-05923
000315516 041__ $$aEnglish
000315516 1001_ $$0P:(DE-HGF)0$$aMuratova, V. N.$$b0
000315516 1112_ $$0C14-06-29.1$$2inspire$$a10th Patras Workshop on Axions, WIMPs and WISPs$$cGeneva$$d2014-06-29 - 2014-07-04$$gAXION-WIMP 2014$$wSwitzerland
000315516 245__ $$aSearches for axioelectric effect of solar axions with BGO-scintillator and BGO-bolometer detectors
000315516 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2014
000315516 29510 $$aMuratova, 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
000315516 300__ $$a117-120
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000315516 520__ $$aA 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..
000315516 7001_ $$0P:(DE-HGF)0$$aDerbin, A. V.$$b1
000315516 7001_ $$0P:(DE-HGF)0$$aGiorni, L.$$b2
000315516 7001_ $$0P:(DE-HGF)0$$aNagorny, S. S$$b3
000315516 7001_ $$0P:(DE-HGF)0$$aPattavina, L.$$b4
000315516 7001_ $$0P:(DE-HGF)0$$aBakhlanov, S. V.$$b5
000315516 7001_ $$0P:(DE-HGF)0$$aBeeman, J. W.$$b6
000315516 7001_ $$0P:(DE-HGF)0$$aBellini, F.$$b7
000315516 7001_ $$0P:(DE-HGF)0$$aBiassoni, M.$$b8
000315516 7001_ $$0P:(DE-HGF)0$$aCapelli, S.$$b9
000315516 7001_ $$0P:(DE-HGF)0$$aClemenza, M.$$b10
000315516 7001_ $$0P:(DE-HGF)0$$aDratchnev, I. S.$$b11
000315516 7001_ $$0P:(DE-HGF)0$$aFerri, E.$$b12
000315516 7001_ $$0P:(DE-HGF)0$$aGiachero, A.$$b13
000315516 7001_ $$0P:(DE-HGF)0$$aGotti, C.$$b14
000315516 7001_ $$0P:(DE-HGF)0$$aKayunov, A. S.$$b15
000315516 7001_ $$0P:(DE-HGF)0$$aMaiano, C.$$b16
000315516 7001_ $$0P:(DE-HGF)0$$aMaino, M.$$b17
000315516 7001_ $$0P:(DE-HGF)0$$aPavan, M.$$b18
000315516 7001_ $$0P:(DE-HGF)0$$aPirro, S.$$b19
000315516 7001_ $$0P:(DE-HGF)0$$aSemenov, D. A.$$b20
000315516 7001_ $$0P:(DE-HGF)0$$aSisti, M.$$b21
000315516 7001_ $$0P:(DE-HGF)0$$aUnzhakov, E. V.$$b22
000315516 7870_ $$0PUBDB-2016-05897$$aTsesmelis, Emmanuel et. al.$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$rDESY-PROC-2014-03$$tProceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) : Geneva, Switzerland, June 29-July 4, 2014
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