1991
DOI: 10.1016/0022-3697(91)90062-5
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Doubly-valent rare-earth ions in halide crystals

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Cited by 228 publications
(10 citation statements)
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“…Previous research attributed a defect emitting at 453 nm in NaBr:Eu 2+ to a EuBr 2 -type precipitate, and emission at 461 nm in NaI:Eu 2+ to a EuI 2 -type precipitate. 14 The emission shown in Figure 5c, supported by the larger bandwidth shown in Figure 5d, might therefore also be attributed to a EuBr 2 - or EuI 2 -type precipitate, or a mixture thereof. The band’s emission center shifts to lower energies with increasing Eu concentration.…”
Section: Results and Discussionmentioning
confidence: 81%
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“…Previous research attributed a defect emitting at 453 nm in NaBr:Eu 2+ to a EuBr 2 -type precipitate, and emission at 461 nm in NaI:Eu 2+ to a EuI 2 -type precipitate. 14 The emission shown in Figure 5c, supported by the larger bandwidth shown in Figure 5d, might therefore also be attributed to a EuBr 2 - or EuI 2 -type precipitate, or a mixture thereof. The band’s emission center shifts to lower energies with increasing Eu concentration.…”
Section: Results and Discussionmentioning
confidence: 81%
“…These emissions are attributed to substitutional defects, where Eu 2+ replaces Na + combined with a charge-compensating defect outside of the first coordinating sphere. 14 Between NaBr and NaI, the only changes in this first coordinating sphere are the type of the anions (becoming more electronegative from Br to I) and the distance of the anions (having a larger ionic radius from Br to I). From a well-mixed phase that follows Vegard’s law we would therefore expect the emission to change fluently from NaBr at 428 nm to NaI at 441 nm, regardless of Eu concentration.…”
Section: Results and Discussionmentioning
confidence: 99%
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