Axion Dark Matter eXperiment: Run 1A analysis details

被引：3

作者：

Boutan, C. ^{[1
]}

Laroque, B. H. ^{[1
]}

Lentz, E. ^{[1
]}

Oblath, N. S. ^{[1
]}

Taubman, M. S. ^{[1
]}

Tedeschi, J. ^{[1
]}

Yang, J. ^{[1
]}

Jones, A. M. ^{[1
,16
]}

Braine, T. ^{[2
]}

Crisosto, N. ^{[2
]}

Rosenberg, L. J. ^{[2
]}

Rybka, G. ^{[2
]}

Will, D. ^{[2
]}

Zhang, D. ^{[2
]}

Kimes, S. ^{[2
,17
]}

Ottens, R. ^{[2
,18
]}

Bartram, C. ^{[3
]}

Bowring, D. ^{[4
]}

Cervantes, R. ^{[4
]}

Chou, A. S. ^{[4
]}

Knirck, S. ^{[4
]}

V. Mitchell, D. ^{[4
]}

Sonnenschein, A. ^{[4
]}

Wester, W. ^{[4
]}

Khatiwada, R. ^{[5
,6
]}

Carosi, G. ^{[7
]}

Du, N. ^{[7
]}

Durham, S. ^{[7
]}

O'Kelley, S. R. ^{[7
]}

Woollett, N. ^{[19
]}

Duffy, L. D. ^{[8
]}

Bradley, R. ^{[9
]}

Clarke, J. ^{[10
]}

Siddiqi, I. ^{[10
]}

Agrawal, A. ^{[11
,20
]}

Dixit, A. V. ^{[11
,21
]}

Gleason, J. R. ^{[12
]}

Hipp, A. T. ^{[12
]}

Jois, S. ^{[12
]}

Sikivie, P. ^{[12
]}

Sullivan, N. S. ^{[12
]}

Tanner, D. B. ^{[12
]}

Buckley, J. H. ^{[13
]}

Gaikwad, C. ^{[13
]}

Henriksen, E. A. ^{[13
]}

Hoffman, J. ^{[13
]}

Murch, K. W. ^{[13
]}

Harrington, P. M. ^{[13
,22
]}

Daw, E. J. ^{[14
]}

Perry, M. G. ^{[14
]}

机构：

[1] Pacific Northwest Natl Lab, Richland, WA 99354 USA

[2] Univ Washington, Seattle, WA 98195 USA

[3] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA

[4] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA

[5] IIT, Chicago, IL 60510 USA

[6] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA

[7] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA

[8] Los Alamos Natl Lab, Los Alamos, NM 87545 USA

[9] Natl Radio Astron Observ, Charlottesville, VA 22903 USA

[10] Univ Calif Berkeley, Berkeley, CA 94720 USA

[11] Univ Chicago, Chicago, IL 60637 USA

[12] Univ Florida, Gainesville, FL 32611 USA

[13] Washington Univ, St Louis, MO 63130 USA

[14] Univ Sheffield, Sheffield S10 2TN, England

[15] Natl Inst Stand & Technol, Gaithersburg, MD 20899 USA

[16] Open Engn Inc, Richland, WA 99354 USA

[17] Microsoft, Microsoft Quantum, Redmond, WA 98052 USA

[18] NASA Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA

[19] Rigetti Comp, Oxford, England

[20] Amazon Web Serv Ctr Quantum Networking, Boston, MA USA

[21] Natl Inst Stand & Technol, Adv Microwave Photon Grp, Gaithersburg, MD 20899 USA

[22] MIT, Res Lab Elect, Cambridge, MA 02139 USA

来源：

PHYSICAL REVIEW D | 2024年 / 109卷 / 11期

关键词：

INVARIANCE;

D O I：

10.1103/PhysRevD.109.012009

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 mu eV 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.

引用

页数：26

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