The nonradiative transition rates Stick to the components WNR = W (0) exp(-alphap), in which p is the number of phonons matching the Power hole. The nonradiative changeover charges of Er3+ exhibit temperature dependence in line with the multiphonon rest concept. In Tm3+ the temperature dependence of nonradiative rest fees https://catep145nlk6.bloggerchest.com/profile