{"paper":{"title":"Search for axioelectric effect of solar axions using BGO scintillating bolometer","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","hep-ph"],"primary_cat":"hep-ex","authors_text":"A. Giachero, A.S. Kayunov, A.V. Derbin, C. Gotti, C. Maiano, D.A. Semenov, E. Ferri, E.V. Unzhakov, F. Bellini, I.S. Drachnev, J.W. Beeman, L. Gironi, L. Pattavina, M. Biassoni, M. Clemenza, M. Maino, M. Pavan, M. Sisti, S. Capelli, S. Pirro, S.S. Nagorny, V.N. Muratova","submitted_at":"2014-05-15T09:48:21Z","abstract_excerpt":"A search for axioelectric absorption of solar axions produced in the $ p + d \\rightarrow {^3\\rm{He}}+\\gamma~(5.5~ \\rm{MeV})$ reactions has been performed with a BGO detector placed in a low-background setup. A model-independent limit on an axion-nucleon and axion-electron coupling constant has been obtained: $| g_{Ae}\\times g_{AN}^3|< 1.9\\times 10^{-10}$ for 90% confidence level. The constrains of the axion-electron coupling have been obtained for hadronic axion with masses in (0.1 - 1) MeV range: $|g_{Ae}| \\leq (0.96 - 8.2)\\times 10^{-8}$."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.3782","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}