Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX

G. Carosi; C. Cisneros; N. Du; S. Durham; N. Robertson; C. Goodman; M. Guzzetti; C. Hanretty; K. Enzian; L. J. Rosenberg; G. Rybka; J. Sinnis; D. Zhang; John Clarke; I. Siddiqi; A. S. Chou; M. Hollister; A. Sonnenschein; S. Knirck; T. J. Caligiure; J. R. Gleason; A. T. Hipp; P. Sikivie; M. E. Solano; N. S. Sullivan; D. B. Tanner; R. Khatiwada; L. D. Duffy; C. Boutan; T. Braine; E. Lentz; N. S. Oblath; M. S. Taubman; E. J. Daw; C. Mostyn; M. G. Perry; C. Bartram; J. Laurel; A. Yi; T. A. Dyson; S. Ruppert; M. O. Withers; C. L. Kuo; B. T. McAllister; J. H. Buckley; C. Gaikwad; J. Hoffman; K. Murch; M. Goryachev; E. Hartman; A. Quiskamp; M. E. Tobar

doi:10.1103/d7mg-6sqq

Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX

G. Carosi
, C. Cisneros
, N. Du
, S. Durham
, N. Robertson
, C. Goodman
, M. Guzzetti
, C. Hanretty
, K. Enzian
, L. J. Rosenberg
, G. Rybka
, J. Sinnis
, D. Zhang
, John Clarke
, I. Siddiqi
, A. S. Chou
, M. Hollister
, A. Sonnenschein
, S. Knirck
, T. J. Caligiure

J. R. Gleason, A. T. Hipp, P. Sikivie, M. E. Solano, N. S. Sullivan, D. B. Tanner, R. Khatiwada, L. D. Duffy, C. Boutan, T. Braine, E. Lentz, N. S. Oblath, M. S. Taubman, E. J. Daw, C. Mostyn, M. G. Perry, C. Bartram, J. Laurel, A. Yi, T. A. Dyson, S. Ruppert, M. O. Withers, C. L. Kuo, B. T. McAllister, J. H. Buckley, C. Gaikwad, J. Hoffman, K. Murch, M. Goryachev, E. Hartman, A. Quiskamp, M. E. Tobar

Research output: Contribution to journal › Article › peer-review

1 Scopus citations

Abstract

Axion dark matter can satisfy the conditions needed to account for all of the dark matter and solve the strong CP problem. The Axion Dark Matter eXperiment (ADMX) is a direct dark matter search using a haloscope to convert axions to photons in an external magnetic field. Key to this conversion is the use of a microwave resonator that enhances the sensitivity at the frequency of interest. The ADMX experiment boosts its sensitivity using a dilution refrigerator and near quantum-limited amplifier to reduce the noise level in the experimental apparatus. In the most recent run, ADMX searched for axions between 1.10 and 1.31 GHz to extended Kim-Shifman-Vainshtein-Zakharov sensitivity. This Letter reports on the results of that run, as well as unique aspects of this experimental setup.

Original language	English
Article number	191001
Journal	Physical Review Letters
Volume	135
Issue number	19
DOIs	https://doi.org/10.1103/d7mg-6sqq
State	Published - Nov 7 2025

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Carosi, G., Cisneros, C., Du, N., Durham, S., Robertson, N., Goodman, C., Guzzetti, M., Hanretty, C., Enzian, K., Rosenberg, L. J., Rybka, G., Sinnis, J., Zhang, D., Clarke, J., Siddiqi, I., Chou, A. S., Hollister, M., Sonnenschein, A., Knirck, S., ... Tobar, M. E. (2025). Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX. Physical Review Letters, 135(19), Article 191001. https://doi.org/10.1103/d7mg-6sqq

@article{5e7468f3a1204a75984cf351454da867,

title = "Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX",

abstract = "Axion dark matter can satisfy the conditions needed to account for all of the dark matter and solve the strong CP problem. The Axion Dark Matter eXperiment (ADMX) is a direct dark matter search using a haloscope to convert axions to photons in an external magnetic field. Key to this conversion is the use of a microwave resonator that enhances the sensitivity at the frequency of interest. The ADMX experiment boosts its sensitivity using a dilution refrigerator and near quantum-limited amplifier to reduce the noise level in the experimental apparatus. In the most recent run, ADMX searched for axions between 1.10 and 1.31 GHz to extended Kim-Shifman-Vainshtein-Zakharov sensitivity. This Letter reports on the results of that run, as well as unique aspects of this experimental setup.",

author = "G. Carosi and C. Cisneros and N. Du and S. Durham and N. Robertson and C. Goodman and M. Guzzetti and C. Hanretty and K. Enzian and Rosenberg, \{L. J.\} and G. Rybka and J. Sinnis and D. Zhang and John Clarke and I. Siddiqi and Chou, \{A. S.\} and M. Hollister and A. Sonnenschein and S. Knirck and Caligiure, \{T. J.\} and Gleason, \{J. R.\} and Hipp, \{A. T.\} and P. Sikivie and Solano, \{M. E.\} and Sullivan, \{N. S.\} and Tanner, \{D. B.\} and R. Khatiwada and Duffy, \{L. D.\} and C. Boutan and T. Braine and E. Lentz and Oblath, \{N. S.\} and Taubman, \{M. S.\} and Daw, \{E. J.\} and C. Mostyn and Perry, \{M. G.\} and C. Bartram and J. Laurel and A. Yi and Dyson, \{T. A.\} and S. Ruppert and Withers, \{M. O.\} and Kuo, \{C. L.\} and McAllister, \{B. T.\} and Buckley, \{J. H.\} and C. Gaikwad and J. Hoffman and K. Murch and M. Goryachev and E. Hartman and A. Quiskamp and Tobar, \{M. E.\}",

note = "Publisher Copyright: {\textcopyright} 2025 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the {"}https://creativecommons.org/licenses/by/4.0/{"}Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Funded by SCOAP3.",

year = "2025",

month = nov,

day = "7",

doi = "10.1103/d7mg-6sqq",

language = "English",

volume = "135",

journal = "Physical Review Letters",

issn = "0031-9007",

number = "19",

}

Carosi, G, Cisneros, C, Du, N, Durham, S, Robertson, N, Goodman, C, Guzzetti, M, Hanretty, C, Enzian, K, Rosenberg, LJ, Rybka, G, Sinnis, J, Zhang, D, Clarke, J, Siddiqi, I, Chou, AS, Hollister, M, Sonnenschein, A, Knirck, S, Caligiure, TJ, Gleason, JR, Hipp, AT, Sikivie, P, Solano, ME, Sullivan, NS, Tanner, DB, Khatiwada, R, Duffy, LD, Boutan, C, Braine, T, Lentz, E, Oblath, NS, Taubman, MS, Daw, EJ, Mostyn, C, Perry, MG, Bartram, C, Laurel, J, Yi, A, Dyson, TA, Ruppert, S, Withers, MO, Kuo, CL, McAllister, BT, Buckley, JH, Gaikwad, C, Hoffman, J, Murch, K, Goryachev, M, Hartman, E, Quiskamp, A & Tobar, ME 2025, 'Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX', Physical Review Letters, vol. 135, no. 19, 191001. https://doi.org/10.1103/d7mg-6sqq

TY - JOUR

T1 - Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX

AU - Carosi, G.

AU - Cisneros, C.

AU - Du, N.

AU - Durham, S.

AU - Robertson, N.

AU - Goodman, C.

AU - Guzzetti, M.

AU - Hanretty, C.

AU - Enzian, K.

AU - Rosenberg, L. J.

AU - Rybka, G.

AU - Sinnis, J.

AU - Zhang, D.

AU - Clarke, John

AU - Siddiqi, I.

AU - Chou, A. S.

AU - Hollister, M.

AU - Sonnenschein, A.

AU - Knirck, S.

AU - Caligiure, T. J.

AU - Gleason, J. R.

AU - Hipp, A. T.

AU - Sikivie, P.

AU - Solano, M. E.

AU - Sullivan, N. S.

AU - Tanner, D. B.

AU - Khatiwada, R.

AU - Duffy, L. D.

AU - Boutan, C.

AU - Braine, T.

AU - Lentz, E.

AU - Oblath, N. S.

AU - Taubman, M. S.

AU - Daw, E. J.

AU - Mostyn, C.

AU - Perry, M. G.

AU - Bartram, C.

AU - Laurel, J.

AU - Yi, A.

AU - Dyson, T. A.

AU - Ruppert, S.

AU - Withers, M. O.

AU - Kuo, C. L.

AU - McAllister, B. T.

AU - Buckley, J. H.

AU - Gaikwad, C.

AU - Hoffman, J.

AU - Murch, K.

AU - Goryachev, M.

AU - Hartman, E.

AU - Quiskamp, A.

AU - Tobar, M. E.

N1 - Publisher Copyright: © 2025 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/"Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Funded by SCOAP3.

PY - 2025/11/7

Y1 - 2025/11/7

N2 - Axion dark matter can satisfy the conditions needed to account for all of the dark matter and solve the strong CP problem. The Axion Dark Matter eXperiment (ADMX) is a direct dark matter search using a haloscope to convert axions to photons in an external magnetic field. Key to this conversion is the use of a microwave resonator that enhances the sensitivity at the frequency of interest. The ADMX experiment boosts its sensitivity using a dilution refrigerator and near quantum-limited amplifier to reduce the noise level in the experimental apparatus. In the most recent run, ADMX searched for axions between 1.10 and 1.31 GHz to extended Kim-Shifman-Vainshtein-Zakharov sensitivity. This Letter reports on the results of that run, as well as unique aspects of this experimental setup.

AB - Axion dark matter can satisfy the conditions needed to account for all of the dark matter and solve the strong CP problem. The Axion Dark Matter eXperiment (ADMX) is a direct dark matter search using a haloscope to convert axions to photons in an external magnetic field. Key to this conversion is the use of a microwave resonator that enhances the sensitivity at the frequency of interest. The ADMX experiment boosts its sensitivity using a dilution refrigerator and near quantum-limited amplifier to reduce the noise level in the experimental apparatus. In the most recent run, ADMX searched for axions between 1.10 and 1.31 GHz to extended Kim-Shifman-Vainshtein-Zakharov sensitivity. This Letter reports on the results of that run, as well as unique aspects of this experimental setup.

UR - https://www.scopus.com/pages/publications/105022740409

U2 - 10.1103/d7mg-6sqq

DO - 10.1103/d7mg-6sqq

M3 - Article

C2 - 41269976

AN - SCOPUS:105022740409

SN - 0031-9007

VL - 135

JO - Physical Review Letters

JF - Physical Review Letters

IS - 19

M1 - 191001

ER -

Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX

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