학술논문
Axion Dark Matter eXperiment: Run 1B Analysis Details
Document Type
Working Paper
Author
ADMX Collaboration; Bartram, C.; Braine, T.; Cervantes, R.; Crisosto, N.; Du, N.; Leum, G.; Rosenberg, L. J; Rybka, G.; Yang, J.; Bowring, D.; Chou, A. S.; Khatiwada, R.; Sonnenschein, A.; Wester, W.; Carosi, G.; Woollett, N.; Duffy, L. D.; Goryachev, M.; McAllister, B.; Tobar, M. E.; Boutan, C.; Jones, M.; Laroque, B. H.; Oblath, N. S.; Taubman, M. S.; Clarke, John; Dove, A.; Eddins, A.; O'Kelley, S. R.; Nawaz, S.; Siddiqi, I.; Stevenson, N.; Agrawal, A.; Dixit, A. V.; Gleason, J. R.; Jois, S.; Sikivie, P.; Solomon, J. A.; Sullivan, N. S.; Tanner, D. B.; Lentz, E.; Daw, E. J.; Perry, M. G.; Buckley, J. H.; Harrington, P. M.; Henriksen, E. A.; Murch, K. W.
Source
Phys. Rev. D 103, 032002 (2021)
Subject
Language
Abstract
Searching for axion dark matter, the ADMX collaboration acquired data from January to October 2018, over the mass range 2.81--3.31 $\mu$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.
Comment: 17 pages, 17 figures
Comment: 17 pages, 17 figures