Cryogenic cavity detector for a large-scale cold dark-matter axion search

被引：46

作者：

Peng, H

Asztalos, S

Daw, E

Golubev, NA

Hagmann, C

Kinion, D

LaVeigne, J

Moltz, DM

Nezrick, F

Powell, J

Rosenberg, LJ

Sikivie, P

Stoeffl, W

Sullivan, NS

Tanner, DB

Turner, MS

van Bibber, K

机构：

[1] MIT, Dept Phys, Cambridge, MA 02139 USA

[2] MIT, Nucl Sci Lab, Cambridge, MA 02139 USA

[3] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia

[4] Univ Calif Lawrence Livermore Natl Lab, Livermore, CA 94550 USA

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

[6] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA

[7] Fermi Natl Accelerator Lab, Batavia, IL 60510 USA

[8] Univ Chicago, Enrico Fermi Inst, Dept Astron & Astrophys, FNAL,NASA Astrophys Ctr, Chicago, IL 60637 USA

[9] Univ Chicago, Enrico Fermi Inst, Dept Phys, FNAL,NASA Astrophys Ctr, Chicago, IL 60637 USA

来源：

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2000年 / 444卷 / 03期

基金：

美国国家科学基金会;

关键词：

axions; dark matter; microwave detector;

D O I：

10.1016/S0168-9002(99)00971-7

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

An axion detector consisting of a tunable high-e cavity, a superconducting magnet, and a superheterodyne receiver with an ultra-low noise pre-amplifier has been built to search for galactic halo axions in the mass range of 1.3-13 mu eV. The detector instrumentation, search process, and data analysis are described. For the first time, this class of detector has reached sufficient sensitivity to detect halo axions with high confidence. (C) 2000 Elsevier Science B.V. All rights reserved.

引用

页码：569 / 583

页数：15

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