New Constraints on Dark Photon Dark Matter with Superconducting Nanowire Detectors in an Optical Haloscope

被引:97
作者
Chiles, Jeff [1 ]
Charaev, Ilya [2 ,3 ]
Lasenby, Robert [4 ]
Baryakhtar, Masha [5 ]
Huang, Junwu [6 ]
Roshko, Alexana [1 ]
Burton, George [1 ]
Colangelo, Marco [2 ]
Van Tilburg, Ken [7 ,8 ]
Arvanitaki, Asimina [6 ]
Nam, Sae Woo [1 ]
Berggren, Karl K. [2 ]
机构
[1] NIST, 325 Broadway, Boulder, CO 80305 USA
[2] MIT, 50 Vassar St, Cambridge, MA 02139 USA
[3] Univ Zurich, CH-8057 Zurich, Switzerland
[4] Stanford Univ, Stanford Inst Theoret Phys, Stanford, CA 94305 USA
[5] Univ Washington, Dept Phys, Seattle, WA 98195 USA
[6] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada
[7] New York Univ CCPP, New York, NY 10003 USA
[8] Flatiron Inst, Ctr Computat Astrophys, New York, NY 10010 USA
基金
美国国家科学基金会;
关键词
EFFICIENCY;
D O I
10.1103/PhysRevLett.128.231802
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Uncovering the nature of dark matter is one of the most important goals of particle physics. Light bosonic particles, such as the dark photon, are well-motivated candidates: they are generally long-lived, weakly interacting, and naturally produced in the early universe. In this work, we report on Light A' Multilayer Periodic Optical SNSPD Target, a proof-of-concept experiment searching for dark photon dark matter in the eV mass range, via coherent absorption in a multilayer dielectric haloscope. Using a superconducting nanowire single-photon detector (SNSPD), we achieve efficient photon detection with a dark count rate of ???6 ?? 10???6 counts/s. We find no evidence for dark photon dark matter in the mass range of ???0.7???0.8 eV with kinetic mixing ?? > 10???12, improving existing limits in ?? by up to a factor of 2. With future improvements to SNSPDs, our architecture could probe significant new parameter space for dark photon and axion dark matter in the meV to 10 eV mass range.
引用
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页数:7
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