Search for Invisible Axion Dark Matter in the 3.3-4.2 μeV Mass Range

被引：204

作者：

Bartram, C. ^{[1
]}

Braine, T. ^{[1
]}

Burns, E. ^{[1
]}

Cervantes, R. ^{[1
]}

Crisosto, N. ^{[1
]}

Du, N. ^{[1
]}

Korandla, H. ^{[1
]}

Leum, G. ^{[1
]}

Mohapatra, P. ^{[1
]}

Nitta, T. ^{[1
]}

Rosenberg, L. J. ^{[1
]}

Rybka, G. ^{[1
]}

Yang, J. ^{[1
]}

Clarke, John ^{[2
]}

Siddiqi, I ^{[2
]}

Agrawal, A. ^{[3
]}

Dixit, A., V ^{[3
]}

Awida, M. H. ^{[4
]}

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

Hollister, M. ^{[4
]}

Knirck, S. ^{[4
]}

Sonnenschein, A. ^{[4
]}

Wester, W. ^{[4
]}

Gleason, J. R. ^{[5
]}

Hipp, A. T. ^{[5
]}

Jois, S. ^{[5
]}

Sikivie, P. ^{[5
]}

Sullivan, N. S. ^{[5
]}

Tanner, D. B. ^{[5
]}

Lentz, E. ^{[6
]}

Khatiwada, R. ^{[4
,7
]}

Carosi, G. ^{[8
]}

Robertson, N. ^{[8
]}

Woollett, N. ^{[8
]}

Duffy, L. D. ^{[9
]}

Boutan, C. ^{[10
]}

Jones, M. ^{[10
]}

LaRoque, B. H. ^{[10
]}

Oblath, N. S. ^{[10
]}

Taubman, M. S. ^{[10
]}

Daw, E. J. ^{[11
]}

Perry, M. G. ^{[11
]}

Buckley, J. H. ^{[12
]}

Gaikwad, C. ^{[12
]}

Hoffman, J. ^{[12
]}

Murch, K. W. ^{[12
]}

Goryachev, M. ^{[13
]}

McAllister, B. T. ^{[13
]}

Quiskamp, A. ^{[13
]}

Thomson, C. ^{[13
]}

机构：

[1] Univ Washington, Seattle, WA 98195 USA

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

[3] Univ Chicago, Chicago, IL 60637 USA

[4] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA

[5] Univ Florida, Gainesville, FL 32611 USA

[6] Univ Gottingen, D-37077 Gottingen, Germany

[7] IIT, Chicago, IL 60616 USA

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

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

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

[11] Univ Sheffield, Sheffield S3 7RH, S Yorkshire, England

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

[13] Univ Western Australia, Perth, WA 6009, Australia

来源：

PHYSICAL REVIEW LETTERS | 2021年 / 127卷 / 26期

关键词：

INVARIANCE;

D O I：

10.1103/PhysRevLett.127.261803

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We report the results from a haloscope search for axion dark matter in the 3.3-4.2 mu eV mass range. This search excludes the axion-photon coupling predicted by one of the benchmark models of "invisible" axion dark matter, the Kim-Shifman-Vainshtein-Zakharov model. This sensitivity is achieved using a largevolume cavity, a superconducting magnet, an ultra low noise Josephson parametric amplifier, and subKelvin temperatures. The validity of our detection procedure is ensured by injecting and detecting blind synthetic axion signals.

引用

页数：6

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