Axion Dark Matter eXperiment: Run 1A Analysis Details
Abstract
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.
Keywords
Cite
@article{arxiv.2312.16668,
title = {Axion Dark Matter eXperiment: Run 1A Analysis Details},
author = {C. Boutan and B. H. LaRoque and E. Lentz and N. S. Oblath and M. S. Taubman and J. Tedeschi and J. Yang and A. M. Jones and T. Braine and N. Crisosto and L. J Rosenberg and G. Rybka and D. Will and D. Zhang and S. Kimes and R. Ottens and C. Bartram and D. Bowring and R. Cervantes and A. S. Chou and S. Knirck and D. V. Mitchell and A. Sonnenschein and W. Wester and R. Khatiwada and G. Carosi and N. Du and S. Durham and S. R. O'Kelley and N. Woollett and L. D. Duffy and R. Bradley and J. Clarke and I. Siddiqi and A. Agrawal and A. V. Dixit and J. R. Gleason and A. T. Hipp and S. Jois and P. Sikivie and N. S. Sullivan and D. B. Tanner and J. H. Buckley and C. Gaikwad and E. A. Henriksen and J. Hoffman and K. W. Murch and P. M. Harrington and E. J. Daw and M. G. Perry and E. J. Daw and M. G. Perry and G. C. Hilton},
journal= {arXiv preprint arXiv:2312.16668},
year = {2023}
}
Comments
27 pages, 19 figures, accepted for publication in PRD