Axion dark matter experiment: Run 1B analysis details

(ADMX Collaboration); M. Goryachev; B. McAllister; M. E. Tobar

doi:10.1103/PhysRevD.103.032002

Axion dark matter experiment: Run 1B analysis details

(ADMX Collaboration)
, M. Goryachev
, B. McAllister
, M. E. Tobar

Physics

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

68 Citations (Scopus)

Abstract

Searching for axion dark matter, the ADMX Collaboration acquired data from January to October 2018, over the mass range 2.81-3.31 μeV, corresponding to the frequency range 680-790 MHz. Using an axion haloscope consisting of a microwave cavity in a strong magnetic field, the ADMX experiment excluded Dine-Fischler-Srednicki-Zhitnisky (DFSZ) axions at 90% confidence level and 100% dark matter density over this entire frequency range, except for a few gaps due to mode crossings. This paper explains the full ADMX analysis for run 1B, motivating analysis choices informed by details specific to this run.

Original language	English
Article number	032002
Journal	Physical Review D
Volume	103
Issue number	3
DOIs	https://doi.org/10.1103/PhysRevD.103.032002
Publication status	Published - 8 Feb 2021

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10.1103/PhysRevD.103.032002

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title = "Axion dark matter experiment: Run 1B analysis details",

abstract = "Searching for axion dark matter, the ADMX Collaboration acquired data from January to October 2018, over the mass range 2.81-3.31 μeV, corresponding to the frequency range 680-790 MHz. Using an axion haloscope consisting of a microwave cavity in a strong magnetic field, the ADMX experiment excluded Dine-Fischler-Srednicki-Zhitnisky (DFSZ) axions at 90\% confidence level and 100\% dark matter density over this entire frequency range, except for a few gaps due to mode crossings. This paper explains the full ADMX analysis for run 1B, motivating analysis choices informed by details specific to this run. ",

author = "\{(ADMX Collaboration)\} and C. Bartram and T. Braine and R. Cervantes and N. Crisosto and N. Du and G. Leum and Rosenberg, \{L. J.\} and G. Rybka and J. Yang and D. Bowring and Chou, \{A. S.\} and R. Khatiwada and A. Sonnenschein and W. Wester and G. Carosi and N. Woollett and Duffy, \{L. D.\} and M. Goryachev and B. McAllister and Tobar, \{M. E.\} and C. Boutan and M. Jones and Laroque, \{B. H.\} and Oblath, \{N. S.\} and Taubman, \{M. S.\} and John Clarke and A. Dove and A. Eddins and O'Kelley, \{S. R.\} and S. Nawaz and I. Siddiqi and N. Stevenson and A. Agrawal and Dixit, \{A. V.\} and Gleason, \{J. R.\} and S. Jois and P. Sikivie and Solomon, \{J. A.\} and Sullivan, \{N. S.\} and Tanner, \{D. B.\} and E. Lentz and Daw, \{E. J.\} and Perry, \{M. G.\} and Buckley, \{J. H.\} and Harrington, \{P. M.\} and Henriksen, \{E. A.\} and Murch, \{K. W.\}",

year = "2021",

month = feb,

day = "8",

doi = "10.1103/PhysRevD.103.032002",

language = "English",

volume = "103",

journal = "Physical Review D",

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publisher = "American Physical Society",

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T2 - Run 1B analysis details

AU - (ADMX Collaboration)

AU - Bartram, C.

AU - Braine, T.

AU - Cervantes, R.

AU - Crisosto, N.

AU - Du, N.

AU - Leum, G.

AU - Rosenberg, L. J.

AU - Rybka, G.

AU - Yang, J.

AU - Bowring, D.

AU - Chou, A. S.

AU - Khatiwada, R.

AU - Sonnenschein, A.

AU - Wester, W.

AU - Carosi, G.

AU - Woollett, N.

AU - Duffy, L. D.

AU - Goryachev, M.

AU - McAllister, B.

AU - Tobar, M. E.

AU - Boutan, C.

AU - Jones, M.

AU - Laroque, B. H.

AU - Oblath, N. S.

AU - Taubman, M. S.

AU - Clarke, John

AU - Dove, A.

AU - Eddins, A.

AU - O'Kelley, S. R.

AU - Nawaz, S.

AU - Siddiqi, I.

AU - Stevenson, N.

AU - Agrawal, A.

AU - Dixit, A. V.

AU - Gleason, J. R.

AU - Jois, S.

AU - Sikivie, P.

AU - Solomon, J. A.

AU - Sullivan, N. S.

AU - Tanner, D. B.

AU - Lentz, E.

AU - Daw, E. J.

AU - Perry, M. G.

AU - Buckley, J. H.

AU - Harrington, P. M.

AU - Henriksen, E. A.

AU - Murch, K. W.

PY - 2021/2/8

Y1 - 2021/2/8

N2 - Searching for axion dark matter, the ADMX Collaboration acquired data from January to October 2018, over the mass range 2.81-3.31 μeV, corresponding to the frequency range 680-790 MHz. Using an axion haloscope consisting of a microwave cavity in a strong magnetic field, the ADMX experiment excluded Dine-Fischler-Srednicki-Zhitnisky (DFSZ) axions at 90% confidence level and 100% dark matter density over this entire frequency range, except for a few gaps due to mode crossings. This paper explains the full ADMX analysis for run 1B, motivating analysis choices informed by details specific to this run.

AB - Searching for axion dark matter, the ADMX Collaboration acquired data from January to October 2018, over the mass range 2.81-3.31 μeV, corresponding to the frequency range 680-790 MHz. Using an axion haloscope consisting of a microwave cavity in a strong magnetic field, the ADMX experiment excluded Dine-Fischler-Srednicki-Zhitnisky (DFSZ) axions at 90% confidence level and 100% dark matter density over this entire frequency range, except for a few gaps due to mode crossings. This paper explains the full ADMX analysis for run 1B, motivating analysis choices informed by details specific to this run.

UR - https://www.scopus.com/pages/publications/85100911801

U2 - 10.1103/PhysRevD.103.032002

DO - 10.1103/PhysRevD.103.032002

M3 - Article

AN - SCOPUS:85100911801

SN - 2470-0010

VL - 103

JO - Physical Review D

JF - Physical Review D

IS - 3

M1 - 032002

ER -

Axion dark matter experiment: Run 1B analysis details

Abstract

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