5 EASY FACTS ABOUT ER:YB:YAB CRYSTAL DESCRIBED

The nonradiative transition fees Stick to the components WNR = W (0) exp(-alphap), where by p is the quantity of phonons matching the Power hole. The nonradiative transition costs of Er3+ show temperature dependence in step with the multiphonon rest idea. In Tm3+ the temperature dependence of nonradiative rest premiums is complex because of the exi