{"paper":{"title":"Constraints on the axion-electron coupling for solar axions produced by Compton process and bremsstrahlung","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","hep-ph"],"primary_cat":"hep-ex","authors_text":"A.S. Kayunov, A.V. Derbin, D.A. Semenov, E.V. Unzhakov, V.N. Muratova","submitted_at":"2011-01-12T08:10:16Z","abstract_excerpt":"The search for solar axions produced by Compton ($\\gamma+e^-\\rightarrow e^-+A$) and bremsstrahlung-like ($e^-+Z \\rightarrow Z+e^-+A$) processes has been performed. The axion flux in the both cases depends on the axion-electron coupling constant. The resonant excitation of low-lying nuclear level of $^{169}\\rm{Tm}$ was looked for: $A+^{169}$Tm $\\rightarrow ^{169}$Tm$^*$ $\\rightarrow ^{169}$Tm $+ \\gamma$ (8.41 keV). The Si(Li) detector and $^{169}$Tm target installed inside the low-background setup were used to detect 8.41 keV $\\gamma$-rays. As a result, a new model independent restriction on th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.2290","kind":"arxiv","version":1},"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"}