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Listening for echo from the stimulated axion decay with the 21 CentiMeter Array
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abstract
The axion is a hypothetical elementary particle that could solve the long-standing strong CP problem in particle physics and the dark matter mystery in the cosmos. Due to the stimulation of the ambient photons, the axion dark matter decay into photons is significantly enhanced so that its echo signal could be detected by terrestrial telescopes. As a pathfinder, we study the expected sensitivity of searching for the axion dark matter in the mass range between $0.41$ and $1.6\mu\text{eV}$ with the 21 CentiMeter Array (21CMA). We aim to cover the whole 21CMA frequency range in two years by using a 1MW emitter. We find that the resulting sensitivity on the axion-photon coupling could surpass other existing limits by about one order of magnitude.
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Cited by 1 Pith paper
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Searching for axion dark matter gegenschein of the Vela supernova remnant with FAST
A 26.4-hour search with FAST finds no axion gegenschein toward Vela, constraining the axion-photon coupling to below about 2e-10 GeV^-1 for axion masses 8.7-9.44 and 10.85-12.01 micro-eV.
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