1989
DOI: 10.1002/pssb.2221560217
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Luminescence Decay Times of the Sb3+, Pb2+, and Bi3+ Ions in Alkaline‐Earth Sulfides

Abstract: The luminescence decay times of TI+-type ions in MgS, CaS, SrS, and B a s are measured as a function of temperature from 4.2 t o 150 K. By applying a three-level model, the energy difference AE between the lower excited states 3T,,(3P,) and 3A1,,(3PO) and the transition probabilities from the two excited states to the ground state 3A1S(3So) are derived. The values of the parameters are compared with each other and with those for alkaline-earth oxides.Die Lumineszenzabklingzeiten von T1+-Typ Ionen in MgS, CaS, … Show more

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Cited by 30 publications
(12 citation statements)
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“…Thus, the decay kinetics of the UV emissions of LuAG:Bi and YAG:Bi is similar to that observed for the triplet emission of Bi 3+ centers in some other hosts (see, e.g., [1,[9][10][11]). It can be described within the phenomenological model used in [1] for Bi 3+ centers in Y 3 Ga 5 O 12 .…”
Section: The Low-temperature Luminescence Decay Kinetics and The Quansupporting
confidence: 79%
“…Thus, the decay kinetics of the UV emissions of LuAG:Bi and YAG:Bi is similar to that observed for the triplet emission of Bi 3+ centers in some other hosts (see, e.g., [1,[9][10][11]). It can be described within the phenomenological model used in [1] for Bi 3+ centers in Y 3 Ga 5 O 12 .…”
Section: The Low-temperature Luminescence Decay Kinetics and The Quansupporting
confidence: 79%
“…Comparison of the data obtained for YAG:Bi in the present paper and for LuAG:Bi by Babin et al (2009) with those reported for the UV emission of Bi 3þ centers in other hosts (see, e.g., Wolfert and Blasse, 1985;Donker et al, 1989;Aceves et al, 1996;Nikl et al, 2005) allows us to conclude that the 5.9 eV and 4.57 eV excitation bands arise from the electronic transitions to the singlet and The intensity of the UV band is decreased 10 times. The spectra are distorted around 2.7 eV due to the contamination of the samples with Ce 3þ ions and the reabsorption of the VIS emission in the z2.7 eV absorption band of Ce 3þ centers.…”
Section: Ultraviolet Luminescencesupporting
confidence: 76%
“…At higher temperatures, the decay time decreases due to the luminescence thermal quenching. Analogous τSC(T) dependences were obtained, e.g., for the triplet emission of Pb 2+ centers in alkali halides [131] and Bi 3+ centers in CaO [85], alkaline-earth sulfides [87], and alkaline-earth fluorides [92]. Emission spectra (normalized) of Lu3Al5O12:Bi and Y3Al5O12:Bi measured at 80 K under different excitations shown in the legends.…”
Section: Characteristics Of the Ultraviolet Luminescencesupporting
confidence: 63%
“…Luminescence properties of all Bi 3+ -doped alkaline-earth oxides [79,84,85,88,89,91,133,[232][233][234][235][236][237][238][239], sulfides [84,[86][87][88][89][90] and fluorides [92] are similar ( Table 1). The triplet emission of Bi 3+ ions in these materials shows the extremely small Stokes shift and FWHM and the extremely large energy D of the spin-orbit splitting of the triplet RES (up to 265 meV in CaF 2 [92]).…”
Section: Discussionmentioning
confidence: 99%