@article{b99a807ba9e14aa6b651fcf9096fa7d5,
title = "Search for Invisible Axion Dark Matter in the 3.3-4.2 μeV Mass Range",
abstract = "We report the results from a haloscope search for axion dark matter in the 3.3-4.2 μeV mass range. This search excludes the axion-photon coupling predicted by one of the benchmark models of {"}invisible{"}axion dark matter, the Kim-Shifman-Vainshtein-Zakharov model. This sensitivity is achieved using a large-volume cavity, a superconducting magnet, an ultra low noise Josephson parametric amplifier, and sub-Kelvin temperatures. The validity of our detection procedure is ensured by injecting and detecting blind synthetic axion signals.",
author = "{(ADMX Collaboration)} and C. Bartram and T. Braine and E. Burns and R. Cervantes and N. Crisosto and N. Du and H. Korandla and G. Leum and P. Mohapatra and T. Nitta and Rosenberg, {L. J.} and G. Rybka and J. Yang and John Clarke and I. Siddiqi and A. Agrawal and Dixit, {A. V.} and Awida, {M. H.} and Chou, {A. S.} and M. Hollister and S. Knirck and A. Sonnenschein and W. Wester and Gleason, {J. R.} and Hipp, {A. T.} and S. Jois and P. Sikivie and Sullivan, {N. S.} and Tanner, {D. B.} and E. Lentz and R. Khatiwada and G. Carosi and N. Robertson and N. Woollett and Duffy, {L. D.} and C. Boutan and M. Jones and Laroque, {B. H.} and Oblath, {N. S.} and Taubman, {M. S.} and Daw, {E. J.} and Perry, {M. G.} and Buckley, {J. H.} and C. Gaikwad and J. Hoffman and Murch, {K. W.} and M. Goryachev and McAllister, {B. T.} and A. Quiskamp and C. Thomson and Tobar, {M. E.}",
note = "Funding Information: This work was supported by the U.S. Department of Energy through Grants No. DE-SC0009800, No. DESC0009723, No. DE-SC0010296, No. DE-SC0010280, No. DE-SC0011665, No. DEFG02-97ER41029, No. DEFG02-96ER40956, No. DEAC52-07NA27344, No. DEC03-76SF00098, and No. DE-SC0017987. Fermilab is a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. Additional support was provided by the Heising-Simons Foundation and by the Lawrence Livermore National Laboratory and Pacific Northwest National Laboratory LDRD offices. UWA participation is funded by the ARC Centre of Excellence for Engineered Quantum Systems, Grant No. CE170100009, Dark Matter Particle Physics, Grant No. CE200100008, and Forrest Research Foundation. The corresponding author is supported by JSPS Overseas Research Fellowships No. 202060305. LLNL Release No. LLNL-JRNL-826807. Publisher Copyright: {\textcopyright} 2021 authors. Published by the American Physical Society.",
year = "2021",
month = dec,
day = "24",
doi = "10.1103/PhysRevLett.127.261803",
language = "English",
volume = "127",
journal = "Physical Review Letters",
issn = "0031-9007",
publisher = "American Physical Society",
number = "26",
}