{"paper":{"title":"Search for non-virialized axions with 3.3-4.2 $\\mu$eV mass at selected resolving powers","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Agrawal, A. M. Jones, A. Quiskamp, A. S. Chou, A. Sonnenschein, A. T. Hipp, A. V. Dixit, B. H. LaRoque, B. T. McAllister, C. Bartram, C. Boutan, C. Gaikwad, C. Goodman, C. Hanretty, C. L. Kuo, D. Bowring, D. B. Tanner, D. Zhang, E. Burns, E. Hartman, E. J. Daw, E. Lentz, G. Carosi, G. Leum, G. Rybka, H. Korandla, I. Siddiqi, J. Brodsky, J. H. Buckley, J. Hoffman, John Clarke, J. R. Gleason, J. Russell, J. Sinnis, J. Yang, K. W. Murch, L. D. Duffy, L. J Rosenberg, M. E. Solano, M. E. Tobar, M. Goryachev, M. G. Perry, M. Guzzetti, M. H. Awida, M. Hollister, M. O. Withers, M. S. Taubman, N. Crisosto, N. Du, N. E. Man, N. Roberston, N. S. Oblath, N. S. Sullivan, N. Woollett, P. Mohapatra, P. Sikivie, R. Cervantes, R. Khatiwada, S. Jois, S. Knirck, S. Lee, S. Ruppert, T. A. Dyson, T. Braine, T. J. Caligiure, T. Nitta, W. Wester, Y. Han","submitted_at":"2024-10-11T19:13:43Z","abstract_excerpt":"The Axion Dark Matter eXperiment is sensitive to narrow axion flows, given axions compose a fraction of the dark matter with a non-negligible local density. Detecting these low-velocity dispersion flows requires a high spectral resolution and careful attention to the expected signal modulation due to Earth's motion. We report an exclusion on the local axion dark matter density in narrow flows of $\\rho_a \\gtrsim 0.03\\,\\mathrm{GeV/cm^3}$ and $\\rho_a \\gtrsim 0.004\\,\\mathrm{GeV/cm^3}$ for Dine-Fischler-Srednicki-Zhitnitski and Kim-Shifman-Vainshtein-Zakharov axion-photon couplings, respectively, o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.09203","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2410.09203/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}