When there are no photons available for the transition, the process is called
non-radiative multi-phonon (NMP) process. Now the transition energy from one
parabolic minimum into the other has to be provided by phonons. Due
to energy conservation, a classical transition at the points is possible,
where the binding energy is zero. This is the case only at the intersection
point1
IP of (D.1) and (D.2). The value between and either
or
then specifies the classical barrier which has to be crossed. Assuming linear
coupling, i.e.
, yields
![]() | (D.5) |
Reinserting (D.5) into (D.2) delivers
With the relaxation energy
![]() | (D.9) |
The forward and reverse rates then read
In Fig. D.2 all derived quantities are depicted. Again