The f-d transition of Ce3+ and Tb3+ in BaBPO5 was studied theoretically using the parametric Hamiltonian model. In order to overcome the difficulty in determining many of the parameter values, we adopted the model-spa...The f-d transition of Ce3+ and Tb3+ in BaBPO5 was studied theoretically using the parametric Hamiltonian model. In order to overcome the difficulty in determining many of the parameter values, we adopted the model-space effective Hamiltonian method to determine the crystal-field parameters and spin-orbit parameters values. The method made use of the energies and eigenvectors, which were obtained from an ab initio calculation using the relativistic self-consistent discrete variational Slater software package (DV-Xα). Other parameters, which were less dependent on host crystals, were taken from published data. The calculated values of parameters were reasonable, and the energy-levels and f-d transition spectra agreed reasonably well with the measured excitation spectra of 5d-4f emission.展开更多
基金Project supported by National Natural Science Foundation of China (10774140, 10874173, 11074245, 11011120083)Foundation of the Education Committee of Chongqing (KJ090523)+1 种基金the Knowledge Innovation Project of the Chinese Academy of Sciences (KJCX2-YW-M11)the Special Foundation for Talents of Anhui Province, China (2007Z021)
文摘The f-d transition of Ce3+ and Tb3+ in BaBPO5 was studied theoretically using the parametric Hamiltonian model. In order to overcome the difficulty in determining many of the parameter values, we adopted the model-space effective Hamiltonian method to determine the crystal-field parameters and spin-orbit parameters values. The method made use of the energies and eigenvectors, which were obtained from an ab initio calculation using the relativistic self-consistent discrete variational Slater software package (DV-Xα). Other parameters, which were less dependent on host crystals, were taken from published data. The calculated values of parameters were reasonable, and the energy-levels and f-d transition spectra agreed reasonably well with the measured excitation spectra of 5d-4f emission.