Search for nonvirialized axions with 3.3 − 4.2 μeV mass at selected resolving powers

ADMX Collaboration; A. Quiskamp; M. Goryachev; E. Hartman; M. E. Tobar; B. T. McAllister

doi:10.1103/rlbt-65rc

Search for nonvirialized axions with 3.3 − 4.2 μeV mass at selected resolving powers

ADMX Collaboration, A. Quiskamp, M. Goryachev, E. Hartman, M. E. Tobar, B. T. McAllister

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

Abstract

The Axion Dark Matter eXperiment is sensitive to narrow axion flows, given axions comprise a fraction of the dark matter with a non-negligible local density. Detecting these low-velocity dispersion flows requires a high spectral resolution and careful attention to the expected signal modulation due to Earth’s motion. We report an exclusion on the local axion dark matter density in narrow flows of ρ_a ≳ 0.03 GeV=cm³ and ρ_a ≳ 0.004 GeV=cm³ for Dine-Fischler-Srednicki-Zhitnitski and Kim-Shifman-Vainshtein-Zakharov axion-photon couplings, respectively, over the mass range 3.3 − 4.2 μeV. Measurements were made at selected resolving powers to allow for a range of possible velocity dispersions.

Original language	English
Article number	L101101
Number of pages	8
Journal	Physical Review D
Volume	112
Issue number	10
DOIs	https://doi.org/10.1103/rlbt-65rc
Publication status	Published - 3 Nov 2025

Funding

Funders	Funder number
ARC Australian Research Council	CE200100008, CE170100009

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10.1103/rlbt-65rc

Cite this

@article{c0b6771850d940a5b520f3569d7b2d4c,

title = "Search for nonvirialized axions with 3.3 − 4.2 μeV mass at selected resolving powers",

abstract = "The Axion Dark Matter eXperiment is sensitive to narrow axion flows, given axions comprise a fraction of the dark matter with a non-negligible local density. Detecting these low-velocity dispersion flows requires a high spectral resolution and careful attention to the expected signal modulation due to Earth{\textquoteright}s motion. We report an exclusion on the local axion dark matter density in narrow flows of ρa ≳ 0.03 GeV=cm3 and ρa ≳ 0.004 GeV=cm3 for Dine-Fischler-Srednicki-Zhitnitski and Kim-Shifman-Vainshtein-Zakharov axion-photon couplings, respectively, over the mass range 3.3 − 4.2 μeV. Measurements were made at selected resolving powers to allow for a range of possible velocity dispersions.",

author = "\{ADMX Collaboration\} and Hipp, \{A. T.\} and A. Quiskamp and Caligiure, \{T. J.\} and Gleason, \{J. R.\} and Y. Han and S. Jois and P. Sikivie and Solano, \{M. E.\} and Sullivan, \{N. S.\} and Tanner, \{D. B.\} and M. Goryachev and E. Hartman and Tobar, \{M. E.\} and McAllister, \{B. T.\} and Duffy, \{L. D.\} and T. Braine and E. Burns and R. Cervantes and N. Crisosto and C. Goodman and M. Guzzetti and C. Hanretty and S. Lee and H. Korandla and G. Leum and P. Mohapatra and T. Nitta and Rosenberg, \{L. J.\} and G. Rybka and J. Sinnis and D. Zhang and C. Bartram and Dyson, \{T. A.\} and Kuo, \{C. L.\} and S. Ruppert and Withers, \{M. O.\} and Awida, \{M. H.\} and D. Bowring and Chou, \{A. S.\} and M. Hollister and S. Knirck and A. Sonnenschein and W. Wester and J. Brodsky and G. Carosi and N. Du and N. Robertson and N. Woollett and C. Boutan and Jones, \{A. M.\} and LaRoque, \{B. H.\} and E. Lentz and Man, \{N. E.\} and Oblath, \{N. S.\} and Taubman, \{M. S.\} and J. Yang and R. Khatiwada and John Clarke and I. Siddiqi and A. Agrawal and Dixit, \{A. V.\} and Daw, \{E. J.\} and Perry, \{M. G.\} and Buckley, \{J. H.\} and C. Gaikwad and J. Hoffman and Murch, \{K. W.\} and J. Russell",

year = "2025",

month = nov,

day = "3",

doi = "10.1103/rlbt-65rc",

language = "English",

volume = "112",

journal = "Physical Review D",

issn = "2470-0010",

publisher = "American Physical Society",

number = "10",

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TY - JOUR

T1 - Search for nonvirialized axions with 3.3 − 4.2 μeV mass at selected resolving powers

AU - ADMX Collaboration

AU - Hipp, A. T.

AU - Quiskamp, A.

AU - Caligiure, T. J.

AU - Gleason, J. R.

AU - Han, Y.

AU - Jois, S.

AU - Sikivie, P.

AU - Solano, M. E.

AU - Sullivan, N. S.

AU - Tanner, D. B.

AU - Goryachev, M.

AU - Hartman, E.

AU - Tobar, M. E.

AU - McAllister, B. T.

AU - Duffy, L. D.

AU - Braine, T.

AU - Burns, E.

AU - Cervantes, R.

AU - Crisosto, N.

AU - Goodman, C.

AU - Guzzetti, M.

AU - Hanretty, C.

AU - Lee, S.

AU - Korandla, H.

AU - Leum, G.

AU - Mohapatra, P.

AU - Nitta, T.

AU - Rosenberg, L. J.

AU - Rybka, G.

AU - Sinnis, J.

AU - Zhang, D.

AU - Bartram, C.

AU - Dyson, T. A.

AU - Kuo, C. L.

AU - Ruppert, S.

AU - Withers, M. O.

AU - Awida, M. H.

AU - Bowring, D.

AU - Chou, A. S.

AU - Hollister, M.

AU - Knirck, S.

AU - Sonnenschein, A.

AU - Wester, W.

AU - Brodsky, J.

AU - Carosi, G.

AU - Du, N.

AU - Robertson, N.

AU - Woollett, N.

AU - Boutan, C.

AU - Jones, A. M.

AU - LaRoque, B. H.

AU - Lentz, E.

AU - Man, N. E.

AU - Oblath, N. S.

AU - Taubman, M. S.

AU - Yang, J.

AU - Khatiwada, R.

AU - Clarke, John

AU - Siddiqi, I.

AU - Agrawal, A.

AU - Dixit, A. V.

AU - Daw, E. J.

AU - Perry, M. G.

AU - Buckley, J. H.

AU - Gaikwad, C.

AU - Hoffman, J.

AU - Murch, K. W.

AU - Russell, J.

PY - 2025/11/3

Y1 - 2025/11/3

N2 - The Axion Dark Matter eXperiment is sensitive to narrow axion flows, given axions comprise a fraction of the dark matter with a non-negligible local density. Detecting these low-velocity dispersion flows requires a high spectral resolution and careful attention to the expected signal modulation due to Earth’s motion. We report an exclusion on the local axion dark matter density in narrow flows of ρa ≳ 0.03 GeV=cm3 and ρa ≳ 0.004 GeV=cm3 for Dine-Fischler-Srednicki-Zhitnitski and Kim-Shifman-Vainshtein-Zakharov axion-photon couplings, respectively, over the mass range 3.3 − 4.2 μeV. Measurements were made at selected resolving powers to allow for a range of possible velocity dispersions.

AB - The Axion Dark Matter eXperiment is sensitive to narrow axion flows, given axions comprise a fraction of the dark matter with a non-negligible local density. Detecting these low-velocity dispersion flows requires a high spectral resolution and careful attention to the expected signal modulation due to Earth’s motion. We report an exclusion on the local axion dark matter density in narrow flows of ρa ≳ 0.03 GeV=cm3 and ρa ≳ 0.004 GeV=cm3 for Dine-Fischler-Srednicki-Zhitnitski and Kim-Shifman-Vainshtein-Zakharov axion-photon couplings, respectively, over the mass range 3.3 − 4.2 μeV. Measurements were made at selected resolving powers to allow for a range of possible velocity dispersions.

UR - https://www.scopus.com/pages/publications/105020902103

U2 - 10.1103/rlbt-65rc

DO - 10.1103/rlbt-65rc

M3 - Article

AN - SCOPUS:105020902103

SN - 2470-0010

VL - 112

JO - Physical Review D

JF - Physical Review D

IS - 10

M1 - L101101

ER -

Search for nonvirialized axions with 3.3 − 4.2 μeV mass at selected resolving powers

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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Search for nonvirialized axions with 3.3 − 4.2 μeV mass at selected resolving powers

Abstract

Funding

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Projects

Centre of Excellence for Dark Matter Particle Physics

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

Cite this