Axions of mass 50–170 μeV can resonantly convert to GHz-regime photons on evolving peanut-shaped surfaces in early BNS inspirals, producing a narrow signal modulated by the GW frequency.
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Resonant Axion-Photon Conversion in the Early Inspiral of Neutron Star Binaries
Axions of mass 50–170 μeV can resonantly convert to GHz-regime photons on evolving peanut-shaped surfaces in early BNS inspirals, producing a narrow signal modulated by the GW frequency.