Gravitational waves induce OAM transitions in photons with probabilities P_l±1 ~ 10^{-17} and P_l±2 ~ 10^{-20}, enabling a proposed wide-band GW detector insensitive to seismic noise.
To provide an analytical solution, we impose the following assumptions: k3 ≫ kg, and k⊥ ≫ kg
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How gravitational waves change photon orbital angular momentum quantum states
Gravitational waves induce OAM transitions in photons with probabilities P_l±1 ~ 10^{-17} and P_l±2 ~ 10^{-20}, enabling a proposed wide-band GW detector insensitive to seismic noise.