4.8 Article

First Results from ABRACADABRA-10 cm: A Search for Sub-μeV Axion Dark Matter

期刊

PHYSICAL REVIEW LETTERS
卷 122, 期 12, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.122.121802

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资金

  1. National Science Foundation [NSF-PHY-1658693, NSF-PHY-1806440, NSF-PHY-1505858, NSF-PHY-1122374]
  2. DOE [DE-SC0019225]
  3. Kavli Institute for Cosmological Physics at the University of Chicago
  4. Miller Institute for Basic Research in Science at the University of California, Berkeley
  5. MIT Undergraduate Research Opportunities in Physics program
  6. Leinweber Graduate Fellowship Program
  7. Simons Foundation
  8. U.S. Department of Energy, Office of Science, Office of Nuclear Physics [DE-FG02-97ER41041, DEFG02-97ER41033]
  9. Office of High Energy Physics [DE-SC-0012567]
  10. University of North Carolina at Chapel Hill
  11. Research Computing group

向作者/读者索取更多资源

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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