{"paper":{"title":"First Searches for Axions and Axion-Like Particles with the LUX Experiment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"A.A. Chiller, A. Bernstein, A. Currie, A. Dobi, A.J. Bailey, A. Lindote, A. Manalaysay, A.St.J. Murphy, B.G. Lenardo, B.N. Edwards, B.P. Tennyson, C. Aquino, C. Chan, C. Chiller, C. Ghag, C.H. Faham, C. Lee, C.M. Ignarra, C. Nehrkorn, C.R. Hall, C. Rhyne, C. Silva, C. Zhang, D. Byram, D.J. Taylor, D. Khaitan, D.M. Mei, D.N. McKinsey, D.P. Hogan, D.Q. Huang, D.R. Tiedt, D.S. Akerib, E. Druszkiewicz, E.K. Pease, E.M. Boulton, E.P. Bernard, F.L.H. Wolfs, F. Neves, H.M. Ara\\'ujo, H.N. Nelson, J.A. Morad, J. Balajthy, J.E. Cutter, J.E.Y. Dobson, J. Mock, J.R. Verbus, J.T. White, J. Xu, K.C. Oliver-Mallory, K.J. Palladino, K. Kamdin, K. Kazkaz, K. O'Sullivan, K.R. Gibson, K.T. Lesko, K. Yazdani, L. Reichhart, L. Tvrznikova, M.C. Carmona-Benitez, M.F. Marzioni, M.G.D. Gilchriese, M. Hanhardt, M. Horn, M.I. Lopes, M. Moongweluwan, M. Solmaz, M.S. Witherell, M. Szydagis, M. Tripathi, N.A. Larsen, P.A. Terman, P. Beltrame, P. Br\\'as, P. Sorensen, R.C. Webb, R.G. Jacobsen, R.J. Gaitskell, R. Knoche, R.L. Mannino, S.A. Hertel, S. Alsum, S.B. Cahn, S. Fiorucci, S.J. Haselschwardt, S.K. Young, S.R. Fallon, S. Shaw, S. Stephenson, S. Uvarov, T.A. Shutt, T.J.R. Davison, T.J. Sumner, T.J. Whitis, T.P. Biesiadzinski, V.M. Gehman, V.N. Solovov, V. Velan, W.C. Taylor, W.H. To, W. Ji, X. Bai","submitted_at":"2017-04-07T17:12:52Z","abstract_excerpt":"The first searches for axions and axion-like particles with the Large Underground Xenon (LUX) experiment are presented. Under the assumption of an axio-electric interaction in xenon, the coupling constant between axions and electrons, gAe is tested, using data collected in 2013 with an exposure totalling 95 live-days $\\times$ 118 kg. A double-sided, profile likelihood ratio statistic test excludes gAe larger than 3.5 $\\times$ 10$^{-12}$ (90% C.L.) for solar axions. Assuming the DFSZ theoretical description, the upper limit in coupling corresponds to an upper limit on axion mass of 0.12 eV/c$^{"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.02297","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"}