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.
Probing the axion–photon coupling with space-based gravitational wave detectors
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Majoron dark matter coupled to photons via a QED anomaly induces oscillatory birefringence that Advanced LIGO, KAGRA, and future interferometers can probe with added optics.
Dynamic LISA/Taiji sensitivity curves exhibit 20% low-frequency variation and 70% directional source-count variation relative to static models, with quadrant patterns at low frequencies.
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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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Probing Majoron Dark Matter with Gravitational Wave Detectors
Majoron dark matter coupled to photons via a QED anomaly induces oscillatory birefringence that Advanced LIGO, KAGRA, and future interferometers can probe with added optics.
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Construction of Sensitivity Curves for Dynamic LISA and Taiji
Dynamic LISA/Taiji sensitivity curves exhibit 20% low-frequency variation and 70% directional source-count variation relative to static models, with quadrant patterns at low frequencies.