Аннотация:Firmly established in astrophysical observations, dark matter evades direct detection in experiments.Axions and axionlike particles are among the leading dark-matter candidates, and numerous attempts todetect them in laboratories have been performed. Here, we propose to advance these efforts substantially,extending the sensitivity for dark-matter axions in the mass range ð38–54Þ μeV down to the axion-photoncouplings g aγγ ≲ ð10−14 − 10−15Þ GeV−1, motivated by generic models of quantum chromodynamicsaxion. Single-photon detectors operating at ultralow temperatures are key elements of the experiment. Theprojected sensitivity will be reached in one year of data taking with magnetic field of (1–10) T, makingCosmological Axion Sarov Haloscope (CASH) the most sensitive haloscope in this mass range