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 (cf. Fig. D.2), (D.6) can be further evaluated to By combining (D.5) and (D.1), can be written as
| (D.9) |
The forward and reverse rates then read
In Fig. D.2 all derived quantities are depicted. Again gives the number of emitted phonons with an energy of . Their product reflects the strength of coupling and hence has a huge impact on the transition rates of the defect states, e.g. a smaller yields a smaller barrier.