The nonradiative transition rates follow the formulation WNR = W (0) exp(-alphap), exactly where p is the quantity of phonons matching the Power hole. The nonradiative transition premiums of Er3+ exhibit temperature dependence according to the multiphonon rest principle. In Tm3+ the temperature dependence of nonradiative leisure costs is complicated https://tomw592kpq0.bloggosite.com/profile