2000
DOI: 10.1007/3-540-44474-2
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Transition Metal and Rare Earth Compounds

Abstract: The use of general descriptive names, registered names, trademarks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use.Cover design: Friedhelm Steinen-Broo, Barcelona; MEDIO, Berlin Typesetting: Fotosatz-Service K6hler GmbH, 97084 Wiirzburg SPIN: 10719407 02/3020 ra -5 4 3 2 1 0 -Printed on acid-free paper

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Cited by 8 publications
(1 citation statement)
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“…It is well established that suitable host material for UCPL should have low intrinsic phonon energy because the phonons (or lattice vibration) of the host can provide non-radiative decay ways to suppress UCPL. 7 Recently, oxides or oxysalts with high chemical stability and low phonon energy, such as Gd 2 O 3 , Y 2 O 3 , YAlO 3 , Y 3 Al 5 O 12 , NaNbO 3 and La(MoO 4 ) 3 etc., existing in the form of nanocrystal, crystal (or polycrystalline) and ceramics 8−24 as the host for UCPL materials have been studied extensively. GdAlO 3 is a perovskite-structured material with good chemical stability and low cutoff phonon energy (∼580 cm −1 ) 25 and hence should be a suitable host for UCPL.…”
mentioning
confidence: 99%
“…It is well established that suitable host material for UCPL should have low intrinsic phonon energy because the phonons (or lattice vibration) of the host can provide non-radiative decay ways to suppress UCPL. 7 Recently, oxides or oxysalts with high chemical stability and low phonon energy, such as Gd 2 O 3 , Y 2 O 3 , YAlO 3 , Y 3 Al 5 O 12 , NaNbO 3 and La(MoO 4 ) 3 etc., existing in the form of nanocrystal, crystal (or polycrystalline) and ceramics 8−24 as the host for UCPL materials have been studied extensively. GdAlO 3 is a perovskite-structured material with good chemical stability and low cutoff phonon energy (∼580 cm −1 ) 25 and hence should be a suitable host for UCPL.…”
mentioning
confidence: 99%