2022
DOI: 10.1016/j.jallcom.2022.166419
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Energy transfer mediated single-phased white light emission in Bi3+-Eu3+ codoped Ba3YGa2O7.5 for WLED

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Cited by 20 publications
(20 citation statements)
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“…The two primary components of the PLE spectrum observed at 613 nm are a wide peak centered at 252 nm and multiple sharp peaks in the 400–500 nm range. The former is attributed to the charge transfer band from the 2p 6 orbital of the O 2– ions to the 4f 6 orbital of the Eu 3+ ions, while the latter is a result of the distinctive 7 F 0 → 5 L 6 and 7 F 0 → 5 D 2 transitions of the Eu 3+ ions 15,32,33 . Under 252 nm light excitation, the LCGO:0.02Eu 3+ sample shows a series of sharp line emissions in the range from 500 to 725 nm.…”
Section: Resultsmentioning
confidence: 98%
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“…The two primary components of the PLE spectrum observed at 613 nm are a wide peak centered at 252 nm and multiple sharp peaks in the 400–500 nm range. The former is attributed to the charge transfer band from the 2p 6 orbital of the O 2– ions to the 4f 6 orbital of the Eu 3+ ions, while the latter is a result of the distinctive 7 F 0 → 5 L 6 and 7 F 0 → 5 D 2 transitions of the Eu 3+ ions 15,32,33 . Under 252 nm light excitation, the LCGO:0.02Eu 3+ sample shows a series of sharp line emissions in the range from 500 to 725 nm.…”
Section: Resultsmentioning
confidence: 98%
“…The former is attributed to the charge transfer band from the 2p 6 orbital of the O 2ions to the 4f 6 orbital of the Eu 3+ ions, while the latter is a result of the distinctive 7 F 0 → 5 L 6 and 7 F 0 → 5 D 2 transitions of the Eu 3+ ions. 15,32,33 Under 252 nm light excitation, the LCGO:0.02Eu 3+ sample shows a series of sharp line emissions in the range from 500 to 725 nm. The distinctive 5 D 1 → 7 F 0 and 5 D 0 → 7 F J (J = 0-4) transitions of the Eu 3+ ions are what cause these emission peaks.…”
Section: 3mentioning
confidence: 99%
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“…Ce 3+ , Eu 2+ , and Bi 3+ are three activators with parity-allowed transitions that can be effectively excited by the n-UV lights and then emit adjustable light in the visible region. Among them, Bi 3+ -doped phosphors can be synthesized without a reducing atmosphere, which is favorable for safety and economics. In addition, Bi 3+ -doped phosphors usually have a larger Stoker shift, which can effectively reduce the reabsorption effect. Therefore, Bi 3+ -doped phosphors have received extensive attention for LED lighting. However, inadequate thermal stability is a significant issue for the Bi 3+ -doped phosphors, as most of them lose more than 30% of their room-temperature emission at 423 K. The serious thermal quenching (TQ) effect greatly limited the practical application of Bi 3+ -doped phosphors in LED lighting, where the chip will inevitably generate heat during operation.…”
Section: Introductionmentioning
confidence: 99%