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Listening for echo from the stimulated axion decay with the 21 CentiMeter Array

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arxiv 2309.06857 v2 pith:EJWNG6PB submitted 2023-09-13 hep-ph astro-ph.COhep-ex

classification hep-phastro-ph.COhep-ex
keywords axiondarkmatterarraycentimeterdecayechoparticle
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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

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Searching for axion dark matter gegenschein of the Vela supernova remnant with FAST

    astro-ph.CO 2025-02 conditional novelty 6.0 of 10

    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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