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A search for cosmological axions has been performed by scanning a frequency region of MHz centered at about GHz, corresponding to an axion mass eV. The QUAX experimental apparatus, a haloscope comprised of a 1-liter volume tunable cavity immersed in an T magnetic field and a quantum-limited detection chain, set limits on the axion-photon coupling at the GeV level. As no signal candidate has been observed, viable hadronic axion models are ruled out in a currently preferred post-inflationary region eV.

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