Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
5437952 | Ceramics International | 2017 | 8 Pages |
Abstract
Aeschynite-type La1âxLnxTiNbO6 (Ln=Ce, Sm, x=0-1) ceramics were prepared via a conventional solid state method. Analysis of X-ray diffraction, Raman, infrared reflectivity spectra and the microstructures revealed a series of composition-induced phase evolution in sequence: monoclinicâcoexistence of monoclinic and orthorhombicâorthorhombic structure, i.e. MâM+OâO. The critical compositions of distinguishing the dominant M or O phase were x=0.15 in La1âxCexTiNbO6 and x=0.10 in La1âxSmxTiNbO6 ceramics, exactly corresponding to the average ionic radius of rare earth ions (IR) ~1.027Â Ã
. The crystal structure and microwave dielectric properties of RETiNbO6 (RE=rare earth) ceramics strongly depended on IR. Near-zero Ïf was achieved in the Ce-sample with x=0.153 (εr=28.9, QÃf=17,275 GHz@6.54 GHz) as well as in the Sm-sample with x=0.098 (εr=28.2, QÃf=19,186 GHz@6.78 GHz). Eventually, RETiNbO6 would form O euxenite (-Ïf), O aeschynite (+Ïf), and M aeschynite (-Ïf), as IR<0.945 Ã
, 0.945Â Ã
Related Topics
Physical Sciences and Engineering
Materials Science
Ceramics and Composites
Authors
Jian Zhang, Ruzhong Zuo,