Axion Dark Matter Experiment: Detailed design and operations

被引：29

作者：

Khatiwada, R. ^{[1
,2
]}

Bowring, D. ^{[3
]}

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

Sonnenschein, A. ^{[4
]}

Wester, W. ^{[4
]}

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

Braine, T. ^{[5
]}

Bartram, C. ^{[5
]}

Cervantes, R. ^{[5
]}

Crisosto, N. ^{[5
]}

Du, N. ^{[5
]}

Rosenberg, L. J. ^{[5
]}

Rybka, G. ^{[5
]}

Yang, J. ^{[5
]}

Will, D. ^{[5
]}

Kimes, S. ^{[5
,17
]}

Carosi, G. ^{[6
]}

Woollett, N. ^{[6
]}

Durham, S. ^{[6
]}

Duffy, L. D. ^{[7
]}

Bradley, R. ^{[8
]}

Boutan, C. ^{[9
]}

Jones, M. ^{[9
]}

LaRoque, B. H. ^{[9
]}

Oblath, N. S. ^{[9
]}

Taubman, M. S. ^{[9
]}

Tedeschi, J. ^{[9
]}

Clarke, John ^{[10
]}

Dove, A. ^{[10
]}

Hashim, A. ^{[10
]}

Siddiqi, I. ^{[10
]}

Stevenson, N. ^{[10
]}

Eddins, A. ^{[10
,18
]}

O'Kelley, S. R. ^{[10
,19
]}

Nawaz, S. ^{[10
,20
]}

Agrawal, A. ^{[11
]}

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

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

Jois, S. ^{[12
]}

Sikivie, P. ^{[12
]}

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

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

Solomon, J. A. ^{[12
,21
]}

Lentz, E. ^{[13
]}

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

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

Buckley, J. H. ^{[15
]}

Harrington, P. M. ^{[15
]}

Henriksen, E. A. ^{[15
]}

Murch, K. W. ^{[15
]}

机构：

[1] IIT, Dept Phys, Chicago, IL 60616 USA

[2] Fermilab Quantum Inst, Fermi Natl Accelerator Lab, Batavia, IL 60510 USA

[3] Fermilab Natl Accelerator Lab, Accelerator Phys Div, Batavia, IL 60510 USA

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

[5] Univ Washington, Dept Phys, Seattle, WA 98195 USA

[6] Lawrence Livermore Natl Lab, Nucl & Chem Sci Div, Livermore, CA 94550 USA

[7] Los Alamos Natl Lab, Accelerators & Elect Grp, Los Alamos, NM 87545 USA

[8] Natl Radio Astron Observ, NRAO Technol Ctr, Charlottesville, VA 22903 USA

[9] Pacific Northwest Natl Lab, Natl Secur Directorate, Richland, WA 99354 USA

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

[11] Univ Chicago, Dept Phys, Chicago, IL 60637 USA

[12] Univ Florida, Dept Phys, Gainesville, FL 32611 USA

[13] Univ Gottingen, Dept Phys, D-37073 Gottingen, Germany

[14] Univ Sheffield, Dept Phys, Sheffield S10 2TN, S Yorkshire, England

[15] Washington Univ, Dept Phys, St Louis, MO 63130 USA

[16] NIST, Phys Measurement Lab, Gaithersburg, MD 20899 USA

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

[18] IBM Almaden Res Ctr, IBM Quantum, San Jose, CA 95120 USA

[19] Lawrence Livermore Natl Lab, Phys Div, Livermore, CA 94550 USA

[20] Global Commun Semicond Inc, Dept Mfg Engn, Torrance, CA 90505 USA

[21] Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27599 USA

来源：

REVIEW OF SCIENTIFIC INSTRUMENTS | 2021年 / 92卷 / 12期

关键词：

QUANTUM INTERFERENCE DEVICE; CP CONSERVATION; DC SQUID; NOISE; AMPLIFICATION; INVARIANCE; AMPLIFIER;

D O I：

10.1063/5.0037857

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

Axion dark matter experiment ultra-low noise haloscope technology has enabled the successful completion of two science runs (1A and 1B) that looked for dark matter axions in the 2.66-3.1 mu eV mass range with Dine-Fischler-Srednicki-Zhitnisky sensitivity [Du et al., Phys. Rev. Lett. 120, 151301 (2018) and Braine et al., Phys. Rev. Lett. 124, 101303 (2020)]. Therefore, it is the most sensitive axion search experiment to date in this mass range. We discuss the technological advances made in the last several years to achieve this sensitivity, which includes the implementation of components, such as the state-of-the-art quantum-noise-limited amplifiers and a dilution refrigerator. Furthermore, we demonstrate the use of a frequency tunable microstrip superconducting quantum interference device amplifier in run 1A, and a Josephson parametric amplifier in run 1B, along with novel analysis tools that characterize the system noise temperature. Published under an exclusive license by AIP Publishing.

引用

页数：19

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