ADMX Axion Dark Matter Bounds around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability

C. Goodman; M. Guzzetti; C. Hanretty; L. J. Rosenberg; G. Rybka; J. Sinnis; D. Zhang; John Clarke; I. Siddiqi; A. S. Chou; M. Hollister; S. Knirck; A. Sonnenschein; T. J. Caligiure; J. R. Gleason; A. T. Hipp; P. Sikivie; M. E. Solano; N. S. Sullivan; D. B. Tanner; R. Khatiwada; G. Carosi; C. Cisneros; N. Du; N. Robertson; N. Woollett; 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; 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/PhysRevLett.134.111002

ADMX Axion Dark Matter Bounds around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability

C. Goodman
, M. Guzzetti
, C. Hanretty
, L. J. Rosenberg
, G. Rybka
, J. Sinnis
, D. Zhang
, John Clarke
, I. Siddiqi
, A. S. Chou
, M. Hollister
, S. Knirck
, A. Sonnenschein
, T. J. Caligiure
, J. R. Gleason
, A. T. Hipp
, P. Sikivie
, M. E. Solano
, N. S. Sullivan
, D. B. Tanner

R. Khatiwada, G. Carosi, C. Cisneros, N. Du, N. Robertson, N. Woollett, 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, 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

23 Citations (Scopus)

Abstract

We report the results of a QCD axion dark matter search with discovery ability for Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axions using an axion haloscope. Sub-Kelvin noise temperatures are reached with an ultralow noise Josephson parametric amplifier cooled by a dilution refrigerator. This work excludes (with a 90% confidence level) DFSZ axions with masses between 3.27 to 3.34 μeV, assuming a standard halo model with a local energy density of 0.45 GeV/cm3 made up 100% of axions.

Original language	English
Article number	111002
Number of pages	7
Journal	Physical Review Letters
Volume	134
Issue number	11
DOIs	https://doi.org/10.1103/PhysRevLett.134.111002
Publication status	Published - 21 Mar 2025

Funding

Funders	Funder number
ARC Australian Research Council	CE170100009, CE200100008

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10.1103/PhysRevLett.134.111002Licence: CC BY

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Goodman, C., Guzzetti, M., Hanretty, C., Rosenberg, L. J., Rybka, G., Sinnis, J., Zhang, D., Clarke, J., Siddiqi, I., Chou, A. S., Hollister, M., Knirck, S., Sonnenschein, A., Caligiure, T. J., Gleason, J. R., Hipp, A. T., Sikivie, P., Solano, M. E., Sullivan, N. S., ... Tobar, M. E. (2025). ADMX Axion Dark Matter Bounds around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability. Physical Review Letters, 134(11), Article 111002. https://doi.org/10.1103/PhysRevLett.134.111002

@article{ad0ebeff3f6f4c9b9dccb6e4d563fea4,

title = "ADMX Axion Dark Matter Bounds around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability",

abstract = "We report the results of a QCD axion dark matter search with discovery ability for Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axions using an axion haloscope. Sub-Kelvin noise temperatures are reached with an ultralow noise Josephson parametric amplifier cooled by a dilution refrigerator. This work excludes (with a 90\% confidence level) DFSZ axions with masses between 3.27 to 3.34 μeV, assuming a standard halo model with a local energy density of 0.45 GeV/cm3 made up 100\% of axions.",

author = "C. Goodman and M. Guzzetti and C. Hanretty 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 S. Knirck and A. Sonnenschein 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 G. Carosi and C. Cisneros and N. Du and N. Robertson and N. Woollett 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 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 = mar,

day = "21",

doi = "10.1103/PhysRevLett.134.111002",

language = "English",

volume = "134",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "11",

}

Goodman, C, Guzzetti, M, Hanretty, C, Rosenberg, LJ, Rybka, G, Sinnis, J, Zhang, D, Clarke, J, Siddiqi, I, Chou, AS, Hollister, M, Knirck, S, Sonnenschein, A, Caligiure, TJ, Gleason, JR, Hipp, AT, Sikivie, P, Solano, ME, Sullivan, NS, Tanner, DB, Khatiwada, R, Carosi, G, Cisneros, C, Du, N, Robertson, N, Woollett, N, Duffy, LD, Boutan, C, Braine, T, Lentz, E, Oblath, NS, Taubman, MS, Daw, EJ, Mostyn, C, Perry, MG, Bartram, C, 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, 'ADMX Axion Dark Matter Bounds around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability', Physical Review Letters, vol. 134, no. 11, 111002. https://doi.org/10.1103/PhysRevLett.134.111002

TY - JOUR

T1 - ADMX Axion Dark Matter Bounds around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability

AU - Goodman, C.

AU - Guzzetti, M.

AU - Hanretty, C.

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 - Knirck, S.

AU - Sonnenschein, A.

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 - Carosi, G.

AU - Cisneros, C.

AU - Du, N.

AU - Robertson, N.

AU - Woollett, N.

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 - 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 - 2025/3/21

Y1 - 2025/3/21

N2 - We report the results of a QCD axion dark matter search with discovery ability for Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axions using an axion haloscope. Sub-Kelvin noise temperatures are reached with an ultralow noise Josephson parametric amplifier cooled by a dilution refrigerator. This work excludes (with a 90% confidence level) DFSZ axions with masses between 3.27 to 3.34 μeV, assuming a standard halo model with a local energy density of 0.45 GeV/cm3 made up 100% of axions.

AB - We report the results of a QCD axion dark matter search with discovery ability for Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axions using an axion haloscope. Sub-Kelvin noise temperatures are reached with an ultralow noise Josephson parametric amplifier cooled by a dilution refrigerator. This work excludes (with a 90% confidence level) DFSZ axions with masses between 3.27 to 3.34 μeV, assuming a standard halo model with a local energy density of 0.45 GeV/cm3 made up 100% of axions.

UR - https://www.scopus.com/pages/publications/105001047935

U2 - 10.1103/PhysRevLett.134.111002

DO - 10.1103/PhysRevLett.134.111002

M3 - Article

AN - SCOPUS:105001047935

SN - 0031-9007

VL - 134

JO - Physical Review Letters

JF - Physical Review Letters

IS - 11

M1 - 111002

ER -

ADMX Axion Dark Matter Bounds around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability

Abstract

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Centre of Excellence for Dark Matter Particle Physics

ARC Centre of Excellence for Engineered Quantum Systems (EQuS 2017)

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ADMX Axion Dark Matter Bounds around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability

Abstract

Funding

Access to Document

Other files and links

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Projects

Centre of Excellence for Dark Matter Particle Physics

ARC Centre of Excellence for Engineered Quantum Systems (EQuS 2017)

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