Limits on axion-like particles from photon-coupling searches are recast as constraints on massive graviton-like particles across lab, astrophysical, and cosmological experiments using analogous Primakoff and Gertsenshtein conversion mechanisms.
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Monitor and Beacon TDI combinations reach g_aγ ~ 10^{-13} GeV^{-1} at high frequencies while Sagnac performs better at low frequencies, with ASTROD-GW probing axion-like dark matter masses down to 10^{-20} eV.
Majoron dark matter with photon coupling fixed by electroweak and neutrino mass scales induces birefringence signals detectable by Advanced LIGO, KAGRA, and future ground-based laser interferometers.
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Bounds on massive graviton-like particles from searches for axion-like particles coupling to photons
Limits on axion-like particles from photon-coupling searches are recast as constraints on massive graviton-like particles across lab, astrophysical, and cosmological experiments using analogous Primakoff and Gertsenshtein conversion mechanisms.
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Detectability of axion-like dark matter for different time-delay interferometry combinations in space-based gravitational wave detectors
Monitor and Beacon TDI combinations reach g_aγ ~ 10^{-13} GeV^{-1} at high frequencies while Sagnac performs better at low frequencies, with ASTROD-GW probing axion-like dark matter masses down to 10^{-20} eV.
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Probing Majoron Dark Matter with Gravitational Wave Detectors
Majoron dark matter with photon coupling fixed by electroweak and neutrino mass scales induces birefringence signals detectable by Advanced LIGO, KAGRA, and future ground-based laser interferometers.
- The structure of multi-axion solutions to the strong CP problem