The stochastic limit approximation method for "rapid" decay is presented, w
here the damping rate gamma is comparable to the system frequency Omega, i.
e., gamma similar to Omega, whereas the usual stochastic limit approximatio
n is applied only to the weak damping situation gamma much less than Omega.
The key formulas for rapid decay are very similar to those for weak dampin
g, but the dynamics are quite different. From a microscopic Hamiltonian, th
e spin-boson model, a Bloch equation containing two independent time scales
is derived. This is a useful method to extract the minimal dissipative dyn
amics at high temperature k(B)T much greater than(h) over bar Omega and the
master equations obtained are of the Lindblad form unlike that of Caldeira
and Leggett. The validity of the method is confirmed by comparing the mast
er equation derived through this method with the exact one.