Axion Dark Matter eXperiment: Run 1B Analysis Details
Cosmology and Nongalactic Astrophysics
2021-02-17 v1 Instrumentation and Methods for Astrophysics
Abstract
Searching for axion dark matter, the ADMX collaboration acquired data from January to October 2018, over the mass range 2.81--3.31 eV, corresponding to the frequency range 680--790 MHz. Using an axion haloscope consisting of a microwave cavity in a strong magnetic field, the ADMX experiment excluded Dine-Fischler-Srednicki-Zhitnisky (DFSZ) axions at 100% dark matter density over this entire frequency range, except for a few gaps due to mode crossings. This paper explains the full ADMX analysis for Run 1B, motivating analysis choices informed by details specific to this run.
Keywords
Cite
@article{arxiv.2010.06183,
title = {Axion Dark Matter eXperiment: Run 1B Analysis Details},
author = {ADMX Collaboration and C. Bartram and T. Braine and R. Cervantes and N. Crisosto and N. Du and G. Leum and L. J Rosenberg and G. Rybka and J. Yang and D. Bowring and A. S. Chou and R. Khatiwada and A. Sonnenschein and W. Wester and G. Carosi and N. Woollett and L. D. Duffy and M. Goryachev and B. McAllister and M. E. Tobar and C. Boutan and M. Jones and B. H. Laroque and N. S. Oblath and M. S. Taubman and John Clarke and A. Dove and A. Eddins and S. R. O'Kelley and S. Nawaz and I. Siddiqi and N. Stevenson and A. Agrawal and A. V. Dixit and J. R. Gleason and S. Jois and P. Sikivie and J. A. Solomon and N. S. Sullivan and D. B. Tanner and E. Lentz and E. J. Daw and M. G. Perry and J. H. Buckley and P. M. Harrington and E. A. Henriksen and K. W. Murch},
journal= {arXiv preprint arXiv:2010.06183},
year = {2021}
}
Comments
17 pages, 17 figures