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2023-12-27
Axion Dark Matter eXperiment: Run 1A Analysis Details
C. BoutanB. H. LaRoqueE. LentzN. S. OblathM. S. TaubmanJ. TedeschiJ. YangA. M. JonesT. BraineN. CrisostoL. J RosenbergG. RybkaD. WillD. ZhangS. KimesR. OttensC. BartramD. BowringR. CervantesA. S. ChouS. KnirckD. V. MitchellA. SonnenscheinW. WesterR. KhatiwadaG. CarosiN. DuS. DurhamS. R. O'KelleyN. WoollettL. D. DuffyR. BradleyJ. ClarkeI. SiddiqiA. AgrawalA. V. DixitJ. R. GleasonA. T. HippS. JoisP. SikivieN. S. SullivanD. B. TannerJ. H. BuckleyC. GaikwadE. A. HenriksenJ. HoffmanK. W. MurchP. M. HarringtonE. J. DawM. G. PerryE. J. DawM. G. PerryG. C. Hilton
文献摘要
The ADMX collaboration gathered data for its Run 1A axion dark matter search from January to June 2017, scanning with an axion haloscope over the frequency range 645-680 MHz (2.66-2.81 ueV in axion mass) at DFSZ sensitivity. The resulting axion search found no axion-like signals comprising all the dark matter in the form of a virialized galactic halo over the entire frequency range, implying lower bound exclusion limits at or below DFSZ coupling at the 90% confidence level. This paper presents expanded details of the axion search analysis of Run 1A, including review of relevant experimental systems, data-taking operations, preparation and interpretation of raw data, axion search methodology, candidate handling, and final axion limits.
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