2019
DOI: 10.1103/physrevlett.122.121802
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First Results from ABRACADABRA-10 cm: A Search for Sub- μeV Axion Dark Matter

Abstract: 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 axion-like particle dark matter is relatively unexplored, particularly at masses ma 1 µeV. ABRACADABRA is a new experimental program to search for axion dark matter over a broad range of masses, 10 −12 ma 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 … Show more

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Cited by 263 publications
(154 citation statements)
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References 58 publications
(79 reference statements)
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“…The central problem in detecting the axion however is that we do not know the frequency, ω m a (1 + v 2 /2) at which the electromagnetic response to the axion field should be monitored. To search for this frequency, haloscopes either enforce a resonance or constructive interference condition for a signal oscillating at ∼ m a (as in e.g., ADMX [116,117], MADMAX [118,119], HAYSTAC [120][121][122][123], CULTASK [124][125][126], OR-GAN [127,128], KLASH [129] and RADES [130]), or are sensitive to a wide bandwidth of frequencies simultaneously (e.g., ABRACADABRA [131][132][133], BEAST [134] and DM-Radio [135]). See Ref.…”
Section: Axion Searchesmentioning
confidence: 99%
“…The central problem in detecting the axion however is that we do not know the frequency, ω m a (1 + v 2 /2) at which the electromagnetic response to the axion field should be monitored. To search for this frequency, haloscopes either enforce a resonance or constructive interference condition for a signal oscillating at ∼ m a (as in e.g., ADMX [116,117], MADMAX [118,119], HAYSTAC [120][121][122][123], CULTASK [124][125][126], OR-GAN [127,128], KLASH [129] and RADES [130]), or are sensitive to a wide bandwidth of frequencies simultaneously (e.g., ABRACADABRA [131][132][133], BEAST [134] and DM-Radio [135]). See Ref.…”
Section: Axion Searchesmentioning
confidence: 99%
“…Such a technique has been fruitfully translated into a vigorous laboratory detection program by some collaborations like ADMX [122][123][124][125][126], YLW [127] and KLASH [128]. A different technique that implements a dielectric haloscope has been implemented by the MADMAX collaboration [129,130], while the ABRACADABRA experiment exploits the coupling of the dark matter axion to a static magnetic field by probing the oscillating magnetic field induced by the particle [131,132]. For thorough reviews on the topic of the QCD axion, we refer the reader to Refs.…”
Section: Axion Physicsmentioning
confidence: 99%
“…The basic approach of Refs. [5][6][7][8][9][10][11][12][13] and similar proposals is to search for those tiny induced electric or magnetic fields, either by using broadband or resonant detection methods. Note that "tiny" means that, for a DM axion with m a ∼ 10 −5 eV and a coupling g aγ ∼ 10 −15 GeV −1 , a 7 T magnetic field induces an E field with a magnitude of the order 10 −13 V/m.…”
Section: Introductionmentioning
confidence: 99%