期刊
PHYSICAL REVIEW LETTERS
卷 122, 期 12, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.122.121802
关键词
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资金
- National Science Foundation [NSF-PHY-1658693, NSF-PHY-1806440, NSF-PHY-1505858, NSF-PHY-1122374]
- DOE [DE-SC0019225]
- Kavli Institute for Cosmological Physics at the University of Chicago
- Miller Institute for Basic Research in Science at the University of California, Berkeley
- MIT Undergraduate Research Opportunities in Physics program
- Leinweber Graduate Fellowship Program
- Simons Foundation
- U.S. Department of Energy, Office of Science, Office of Nuclear Physics [DE-FG02-97ER41041, DEFG02-97ER41033]
- Office of High Energy Physics [DE-SC-0012567]
- University of North Carolina at Chapel Hill
- Research Computing group
The axion is a promising dark matter candidate, which was originally proposed to solve the strong-CP problem in particle physics. To date, the available parameter space for axion and axionlike particle dark matter is relatively unexplored, particularly at masses m(a) less than or similar to 1 mu eV. ABRACADABRA is a new experimental program to search for axion dark matter over a broad range of masses, 10(-12) less than or similar to m(a) less than or similar to 10(-6) eV. ABRACADABRA-10 cm is a small-scale prototype for a future detector that could be sensitive to the QCD axion. In this Letter, we present the first results from a 1 month search for axions with ABRACADABRA-10 cm. We find no evidence for axionlike cosmic dark matter and set 95% C.L. upper limits on the axion-photon coupling between g(a gamma gamma) < 1.4 x 10(-10) and g(a gamma gamma) < 3.3 x 10(-9) GeV-1 over the mass range 3.1 x 10(-10)-8.3 x 10(-9) eV. These results are competitive with the most stringent astrophysical constraints in this mass range.
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