Axion Dark Matter eXperiment: Run 1A analysis details

C. Boutan; B. H. Laroque; E. Lentz; N. S. Oblath; M. S. Taubman; J. Tedeschi; J. Yang; A. M. Jones; T. Braine; N. Crisosto; L. J. Rosenberg; G. Rybka; D. Will; D. Zhang; S. Kimes; R. Ottens; C. Bartram; D. Bowring; R. Cervantes; A. S. Chou; S. Knirck; D. V. Mitchell; A. Sonnenschein; W. Wester; R. Khatiwada; G. Carosi; N. Du; S. Durham; S. R. O'Kelley; N. Woollett; L. D. Duffy; R. Bradley; J. Clarke; I. Siddiqi; A. Agrawal; A. V. Dixit; J. R. Gleason; A. T. Hipp; S. Jois; P. Sikivie; N. S. Sullivan; D. B. Tanner; J. H. Buckley; C. Gaikwad; E. A. Henriksen; J. Hoffman; K. W. Murch; P. M. Harrington; E. J. Daw; M. G. Perry; G. C. Hilton

doi:10.1103/PhysRevD.109.012009

Axion Dark Matter eXperiment: Run 1A analysis details

C. Boutan
, B. H. Laroque
, E. Lentz
, N. S. Oblath
, M. S. Taubman
, J. Tedeschi
, J. Yang
, A. M. Jones
, T. Braine
, N. Crisosto
, L. J. Rosenberg
, G. Rybka
, D. Will
, D. Zhang
, S. Kimes
, R. Ottens
, C. Bartram
, D. Bowring
, R. Cervantes
, A. S. Chou

S. Knirck, D. V. Mitchell, A. Sonnenschein, W. Wester, R. Khatiwada, G. Carosi, N. Du, S. Durham, S. R. O'Kelley, N. Woollett, L. D. Duffy, R. Bradley, J. Clarke, I. Siddiqi, A. Agrawal, A. V. Dixit, J. R. Gleason, A. T. Hipp, S. Jois, P. Sikivie, N. S. Sullivan, D. B. Tanner, J. H. Buckley, C. Gaikwad, E. A. Henriksen, J. Hoffman, K. W. Murch, P. M. Harrington, E. J. Daw, M. G. Perry, G. C. Hilton

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

4 Scopus citations

Abstract

The ADMX Collaboration gathered data for its Run 1A axion dark matter search from January 2017 to June 2017, scanning with an axion haloscope over the frequency range 645-680 MHz (2.66-2.81 μeV in axion mass) at Dine-Fischler-Srednicki-Zhitnitskii (DFSZ) sensitivity. The resulting axion search found no axionlike signals comprising all the dark matter in the form of a virialized galactic halo over the entire frequency range, implying lower bound exclusion limits at or below DFSZ coupling at the 90% confidence level. This paper presents expanded details of the axion search analysis of Run 1A, including review of relevant experimental systems, data-taking operations, preparation and interpretation of raw data, axion search methodology, candidate handling, and final axion limits.

Original language	English
Article number	012009
Journal	Physical Review D
Volume	109
Issue number	1
DOIs	https://doi.org/10.1103/PhysRevD.109.012009
State	Published - Jan 1 2024

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10.1103/PhysRevD.109.012009

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Boutan, C., Laroque, B. H., Lentz, E., Oblath, N. S., Taubman, M. S., Tedeschi, J., Yang, J., Jones, A. M., Braine, T., Crisosto, N., Rosenberg, L. J., Rybka, G., Will, D., Zhang, D., Kimes, S., Ottens, R., Bartram, C., Bowring, D., Cervantes, R., ... Hilton, G. C. (2024). Axion Dark Matter eXperiment: Run 1A analysis details. Physical Review D, 109(1), Article 012009. https://doi.org/10.1103/PhysRevD.109.012009

@article{338f0838b37d43a486ac393c97d652c8,

title = "Axion Dark Matter eXperiment: Run 1A analysis details",

abstract = "The ADMX Collaboration gathered data for its Run 1A axion dark matter search from January 2017 to June 2017, scanning with an axion haloscope over the frequency range 645-680 MHz (2.66-2.81 μeV in axion mass) at Dine-Fischler-Srednicki-Zhitnitskii (DFSZ) sensitivity. The resulting axion search found no axionlike signals comprising all the dark matter in the form of a virialized galactic halo over the entire frequency range, implying lower bound exclusion limits at or below DFSZ coupling at the 90\% confidence level. This paper presents expanded details of the axion search analysis of Run 1A, including review of relevant experimental systems, data-taking operations, preparation and interpretation of raw data, axion search methodology, candidate handling, and final axion limits.",

author = "C. Boutan and Laroque, \{B. H.\} and E. Lentz and Oblath, \{N. S.\} and Taubman, \{M. S.\} and J. Tedeschi and J. Yang and Jones, \{A. M.\} and T. Braine and N. Crisosto and Rosenberg, \{L. J.\} and G. Rybka and D. Will and D. Zhang and S. Kimes and R. Ottens and C. Bartram and D. Bowring and R. Cervantes and Chou, \{A. S.\} and S. Knirck and Mitchell, \{D. V.\} and A. Sonnenschein and W. Wester and R. Khatiwada and G. Carosi and N. Du and S. Durham and O'Kelley, \{S. R.\} and N. Woollett and Duffy, \{L. D.\} and R. Bradley and J. Clarke and I. Siddiqi and A. Agrawal and Dixit, \{A. V.\} and Gleason, \{J. R.\} and Hipp, \{A. T.\} and S. Jois and P. Sikivie and Sullivan, \{N. S.\} and Tanner, \{D. B.\} and Buckley, \{J. H.\} and C. Gaikwad and Henriksen, \{E. A.\} and J. Hoffman and Murch, \{K. W.\} and Harrington, \{P. M.\} and Daw, \{E. J.\} and Perry, \{M. G.\} and Hilton, \{G. C.\}",

note = "Publisher Copyright: {\textcopyright} 2024 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 = "2024",

month = jan,

day = "1",

doi = "10.1103/PhysRevD.109.012009",

language = "English",

volume = "109",

journal = "Physical Review D",

issn = "2470-0010",

number = "1",

}

Boutan, C, Laroque, BH, Lentz, E, Oblath, NS, Taubman, MS, Tedeschi, J, Yang, J, Jones, AM, Braine, T, Crisosto, N, Rosenberg, LJ, Rybka, G, Will, D, Zhang, D, Kimes, S, Ottens, R, Bartram, C, Bowring, D, Cervantes, R, Chou, AS, Knirck, S, Mitchell, DV, Sonnenschein, A, Wester, W, Khatiwada, R, Carosi, G, Du, N, Durham, S, O'Kelley, SR, Woollett, N, Duffy, LD, Bradley, R, Clarke, J, Siddiqi, I, Agrawal, A, Dixit, AV, Gleason, JR, Hipp, AT, Jois, S, Sikivie, P, Sullivan, NS, Tanner, DB, Buckley, JH, Gaikwad, C, Henriksen, EA, Hoffman, J, Murch, KW, Harrington, PM, Daw, EJ, Perry, MG & Hilton, GC 2024, 'Axion Dark Matter eXperiment: Run 1A analysis details', Physical Review D, vol. 109, no. 1, 012009. https://doi.org/10.1103/PhysRevD.109.012009

TY - JOUR

T1 - Axion Dark Matter eXperiment

T2 - Run 1A analysis details

AU - Boutan, C.

AU - Laroque, B. H.

AU - Lentz, E.

AU - Oblath, N. S.

AU - Taubman, M. S.

AU - Tedeschi, J.

AU - Yang, J.

AU - Jones, A. M.

AU - Braine, T.

AU - Crisosto, N.

AU - Rosenberg, L. J.

AU - Rybka, G.

AU - Will, D.

AU - Zhang, D.

AU - Kimes, S.

AU - Ottens, R.

AU - Bartram, C.

AU - Bowring, D.

AU - Cervantes, R.

AU - Chou, A. S.

AU - Knirck, S.

AU - Mitchell, D. V.

AU - Sonnenschein, A.

AU - Wester, W.

AU - Khatiwada, R.

AU - Carosi, G.

AU - Du, N.

AU - Durham, S.

AU - O'Kelley, S. R.

AU - Woollett, N.

AU - Duffy, L. D.

AU - Bradley, R.

AU - Clarke, J.

AU - Siddiqi, I.

AU - Agrawal, A.

AU - Dixit, A. V.

AU - Gleason, J. R.

AU - Hipp, A. T.

AU - Jois, S.

AU - Sikivie, P.

AU - Sullivan, N. S.

AU - Tanner, D. B.

AU - Buckley, J. H.

AU - Gaikwad, C.

AU - Henriksen, E. A.

AU - Hoffman, J.

AU - Murch, K. W.

AU - Harrington, P. M.

AU - Daw, E. J.

AU - Perry, M. G.

AU - Hilton, G. C.

N1 - Publisher Copyright: © 2024 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 - 2024/1/1

Y1 - 2024/1/1

N2 - The ADMX Collaboration gathered data for its Run 1A axion dark matter search from January 2017 to June 2017, scanning with an axion haloscope over the frequency range 645-680 MHz (2.66-2.81 μeV in axion mass) at Dine-Fischler-Srednicki-Zhitnitskii (DFSZ) sensitivity. The resulting axion search found no axionlike signals comprising all the dark matter in the form of a virialized galactic halo over the entire frequency range, implying lower bound exclusion limits at or below DFSZ coupling at the 90% confidence level. This paper presents expanded details of the axion search analysis of Run 1A, including review of relevant experimental systems, data-taking operations, preparation and interpretation of raw data, axion search methodology, candidate handling, and final axion limits.

AB - The ADMX Collaboration gathered data for its Run 1A axion dark matter search from January 2017 to June 2017, scanning with an axion haloscope over the frequency range 645-680 MHz (2.66-2.81 μeV in axion mass) at Dine-Fischler-Srednicki-Zhitnitskii (DFSZ) sensitivity. The resulting axion search found no axionlike signals comprising all the dark matter in the form of a virialized galactic halo over the entire frequency range, implying lower bound exclusion limits at or below DFSZ coupling at the 90% confidence level. This paper presents expanded details of the axion search analysis of Run 1A, including review of relevant experimental systems, data-taking operations, preparation and interpretation of raw data, axion search methodology, candidate handling, and final axion limits.

UR - https://www.scopus.com/pages/publications/85183842269

U2 - 10.1103/PhysRevD.109.012009

DO - 10.1103/PhysRevD.109.012009

M3 - Article

AN - SCOPUS:85183842269

SN - 2470-0010

VL - 109

JO - Physical Review D

JF - Physical Review D

IS - 1

M1 - 012009

ER -

Axion Dark Matter eXperiment: Run 1A analysis details

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