Synthesis, characterization and fluorescence of N,N'-BIS (6-metyl-2-pyridine-carboxylamide-N-oxide)-1,2-ethane and corresponding rare earth (III) complexes
A new ligand, N,N-BIS (6-metyl-2-pyridinecarboxylamide-N-oxide)-1,2-ethane (L) and six lanthanide(III) complexes (RE=La, Sm, Eu, Tb, Gd, Yb) were synthesized and characterized in detail. The results indicated that the composition of the binary complexes was determined as [REL(H 2O)(NO 3) 2]NO 3· nH...
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Published in | Journal of rare earths Vol. 27; no. 5; pp. 790 - 796 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
Elsevier B.V
01.10.2009
College of Chemistry and Chemical Engineering, Lanzhou University, Lanzhou 730000, China%Department of Chemistry and life Science, Hezuo Minorities Teachers' College, Hezuo 747000, China%College of Chemistry and Chemical Engineering, Lanzhou University, Lanzhou 730000, China Department of Chemistry and life Science, Hezuo Minorities Teachers' College, Hezuo 747000, China |
Subjects | |
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Summary: | A new ligand, N,N-BIS (6-metyl-2-pyridinecarboxylamide-N-oxide)-1,2-ethane (L) and six lanthanide(III) complexes (RE=La, Sm, Eu, Tb, Gd, Yb) were synthesized and characterized in detail. The results indicated that the composition of the binary complexes was determined as [REL(H
2O)(NO
3)
2]NO
3·
nH
2O (
n=0–2), and the Eu
3+ complex had bright red fluorescence in solid state. Three complexes of Eu
3+, Tb
3+, and Gd
3+ with 6-methylpicolinic acid N-oxide (L') were also synthesized. The relative intensity of sensitized luminescence for Eu
3+ increased in the following order: L>L'. The phosphorescence spectra of the Gd
3+ complexes at 77 K were measured. The energies of excited triplet state for the ligands were 20704 cm
−1 (L) and 20408 cm
−1 (L'). The facts that the ligands sensitized Eu
3+ strongly and the order of the emission intensity for Eu
3+ complexes were explained by Δ
E(T-
5D). This meant that the triplet energy level of the ligand was the main factor to influence RE
3+ luminescence. |
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Bibliography: | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 |
ISSN: | 1002-0721 2509-4963 |
DOI: | 10.1016/S1002-0721(08)60336-1 |