We employ the Schwinger-Keldysh formalism to study the nonequilibrium dynamics of the mirror with perfect reflection moving in a quantum field. In the case where the mirror undergoes the small displacement, the coarse-grained effective action is obtained by integrating out the quantum field with the method of influence functional. The semiclassical Langevin equation is derived, and is found to involve two levels of backreaction effects on the dynamics of mirrors: radiation reaction induced by the motion of the mirror and backreaction dissipation arising from fluctuations in quantum field via a fluctuation-dissipation relation. Although the corresponding theorem of fluctuation and dissipation for the case with the small mirror's displacement is of model independence, the study from the first principles derivation shows that the theorem is also independent of the regulators introduced to deal with short-distance divergences from the quantum field. Thus, when the method of regularization is introduced to compute the dissipation and fluctuation effects, this theorem must be fulfilled as the results are obtained by taking the short-distance limit in the end of calculations. The backreaction effects from vacuum fluctuations on moving mirrors are found to be hardly detected while those effects from thermal fluctuations may be detectable.Zero-point fluctuations due to the imposition of the boundary conditions can lead to an impact on macroscopic physics. One of the most celebrated examples is the attractive Casimir force between two parallel conducting plates [1]. However, the dynamics of fluctuations subject to the moving boundary may also be detectable, sometimes referred to as the dynamical Casimir effects [2,3,4,5,6,7,8,9]. Consider a perfectly reflecting mirror moving in quantum fields. The boundary conditions on quantum fields corresponding to perfect reflection result in the interaction of the mirror with the fields. The motion of the mirror, which leads to the moving boundary, can create quantum radiation that in turn damps out the motion of the mirror as a result of the motion-induced radiation reaction force. In fact, as required by Lorentz invariance of quantum fields, this radiation reaction force vanishes for a motion with uniform velocity. In a motion of uniform acceleration, the mirror suffers from the same fluctuations as if it was at rest in a thermal bath due to the Unruh effects [10], also leading to the zero dissipative radiation reaction force. Fulling and Davies have computed this force for a moving mirror in a massless scalar field in the 1+1 dimensional spacetime. It turns out that the induced dissipative force is proportional to the third time derivative of the mirror's position [7]. In 3+1 dimensional spacetime, the problem has been studied by Ford and Vilenkin in terms of a first order approximation of the mirror's displacement. The corresponding dissipative force then is given by the fifth time derivative of the position in the non-relativistic limit [8]. However, as we know, all quantum field...