1.3 Optical properties
1.3.4 Energy transfer: origin of concentration quenching
When the excitation energy is absorbed by the system (e.g. Eu2O3 and Tb2O3), all the Eu3+/Tb3+ ions within the system do not absorb the energy. The ions that absorb the excitation energy are in the excited state, but the energy is not confined to those ions (excited state). The excitation energy can be transferred from one Eu3+/Tb3+ ion
Figure 1.9: Schematic energy level diagram of Gd2O3with emission transitions. The lowest- energy emission transition (6P7/2 →8S7/2) corresponds to an emission peak in UV (∼ 313 nm) region.
(excited state) to the other Eu3+/Tb3+ ion (ground state). Energy transfer between the two ions is possible only if (a) the energy differences between the ground state and excited state of the two ions are equal, which is known as energy resonance and (b) a suitable interaction between the two ions is present. The interaction between the two ions may be of exchange type (overlap of wave functions) or an electric or magnetic multipolar type.
The electric multipolar interaction is strong if the electric-multipole transitions are allowed.
Since the electric-dipole transitions within the 4f energy levels of Eu3+/Tb3+ ions are forced, but not allowed, the multipolar interactions are weak. Energy transfer between the Eu3+/Tb3+ ions is possible only if the exchange interaction is strong. The strength of the exchange interaction is influenced by the distance between the ions. Typically, the exchange interaction is effective when the distance between the ions is shorter than 5-8 ˚A. At high concentration of the ions (e.g. Eu2O3 and Tb2O3), the distance between them is short. Since the two identical Eu3+/Tb3+ions fulfill the energy resonance criterion and the exchange interaction is effective, the energy transfer occurs. Considering the long radiative lifetimes (∼1 ms) of Eu3+and Tb3+ions, the energy transfer can occur multiple times. The excitation energy can relocate far away from the original location where it was absorbed, which is called energy migration. If the excitation energy migrates to a defect or impurity site where it is lost non-radiatively, the radiative emission (luminescence) is quenched. This process leads to reduction in the luminescence efficiency. This phenomenon is defined as concentration-dependent luminescence quenching or concentration quenching. A schematic of the energy migration process that leads to concentration quenching is shown in figure 1.10.
The Eu3+/Tb3+-doped RE2O3 is preferred over the pure Eu2O3/Tb2O3 for their higher luminescence efficiency. Common host lattices are Y2O3 (lattice constant = 10.60
˚A, space group: Ia3) and Gd2O3 (lattice constant: 10.81 ˚A, space group: Ia3). The crystal structure of these host lattices is identical to that of Eu2O3 and Tb2O3. Typically, Y2O3 is employed because yttrium (Y) is abundant compared to gadolinium (Gd). Reducing
Figure 1.10: Schematic of excitation migration mechanism.
the concentration of luminescent ions minimizes the exchange interaction between them.
For example, all lattice sites occupying RE3+ ions are filled by Eu3+ ions in pure Eu2O3. In contrast, 10%Eu3+:Gd2O3 has only 10% of the RE3+ ion occupying lattice sites filled by Eu3+ ions. The Eu3+ ions occupy these lattice sites in a statistical way. Hence, the Eu3+-Eu3+distance increases as the Eu3+ion concentration decreases, which minimizes the exchange interaction between them at low concentration. The excitation energy migration is reduced and it is confined to the ion where it was absorbed. Thus, the luminescence efficiency is increased.
Low concentration of luminescent ions is required to enhance the luminescence effi- ciency, but a certain concentration should be employed to quench higher energy-level emis- sion transitions by cross-relaxation. In cross-relaxation, a part of the excitation energy of one luminescent ion is transferred to another identical luminescent ion via phonon-assisted energy transfer. Cross-relaxation is the preferred energy transfer mechanism because cer- tain higher energy level emission transitions are quenched at the expense of lower energy level excitation transitions, which can be easily explained for Eu3+ and Tb3+ ions. Fig- ure 1.11 shows cross-relaxation process using the energy level diagrams of Eu3+ and Tb3+
ions. For example, the 5D1 → 5D0 emission transition is quenched in one Eu3+ ion at the
Figure 1.11: Schematic of cross-relaxation mechanism in Eu3+ and Tb3+ ions. The 5D1
→ 5D0 emission transition is quenched in one Eu3+ ion at the expense of the 7F0 → 7F3 excitation transition in another Eu3+ ion. Similarly, the5D3 → 5D4 emission transition is quenched in one Tb3+ ion at the expense of the7F6 →7F0 excitation transition in another Tb3+ ion.
expense of the7F0 → 7F3 excitation transition in another Eu3+ ion. Such transitions are preferred because electrons are populated at the5D0 energy level and emission transitions from the higher energy level [5D1 → 7FJ (J = 0-6)] are avoided. Similarly, the5D3 →5D4 emission transition is quenched in one Tb3+ ion at the expense of the7F6 →7F0 excitation transition in another Tb3+ ion. Thus, electrons are populated at the 5D4 energy level and emission transitions from the higher energy level [5D3 → 7FJ (J = 6-0)] are avoided. The cross-relaxation is observed above a critical concentration of luminescent ions as it depends on the interaction between the luminescent ions. The critical concentration depends on the host lattice (3% Eu3+-doped Y2O3).5 Doping of the host lattice with the luminescent ions to the critical concentration is desired. Doping of the luminescent ions in the host lattice above the critical concentration results in lower luminescence efficiency as described earlier.