Theoretical Detailed Analyses for DC readout and a Fabri-Pérot gravitational-wave detector

The quantum expectation value and the stationary noise spectral density for a Fabri-Pérot gravitational-wave detector with a DC readout scheme are discussed in detail only through the quantum electrodynamics of lasers and the Heisenberg equations of mirrors' motion. We demonstrate that the initial conditions of the mirrors' motion concentrate around the fundamental frequency of the pendulum and are not related to the frequency range of our interest. Although in the ideal case, there is a consensus that the shot noise for the laser in the high-frequency range in the signal-referred noise spectral density decreases if the injected laser power is increased, our obtained noise spectral density shows that the shot noise does not decrease even if the injected laser power is increased. This is due to the leakage of the classical radiation pressure forces from the classical carrier field to the output port, and the classical carrier field is used as the reference in the DC readout scheme. Since the classical radiation pressure forces affect the mirror motion as a classical constant force, this classical constant force changes the equilibrium point of the pendulum of mirrors' motion. To recover the ideal case, we must consider adjusting the interferometer's tuning point to place the mirrors in equilibrium points. We investigate the case where the equilibrium tuning is incomplete and show that the behavior of the above shot noise is due to this incompleteness. We also discuss the maximal deviation of the mirror displacements from the equilibrium point in the incomplete tuning to recover the near ideal case.