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© 2022 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.

Abstract

(Nb5+, Si4+) co-doped TiO2 (NSTO) ceramics with the compositions (Nb0.5Si0.5)xTi1−xO2, x = 0, 0.025, 0.050 and 0.1 were prepared with a solid-state reaction technique. X-ray diffraction (XRD) patterns and Raman spectra confirmed that the tetragonal rutile is the main phase in all the ceramics. Additionally, XRD revealed the presence of a secondary phase of SiO2 in the co-doped ceramics. Impedance spectroscopy analysis showed two contributions, which correspond to the responses of grain and grain-boundary. All the (Nb, Si) co-doped TiO2 showed improved dielectric performance in the high frequency range (>103 Hz). The sample (Nb0.5Si0.5)0.025Ti0.975O2 showed the best dielectric performance in terms of higher relative permittivity (5.5 × 104) and lower dielectric loss (0.18), at 10 kHz and 300 K, compared to pure TiO2 (1.1 × 103, 0.34). The colossal permittivity of NSTO ceramics is attributed to an internal barrier layer capacitance (IBLC) effect, formed by insulating grain-boundaries and semiconductor grains in the ceramics.

Details

Title
Colossal Permittivity Characteristics of (Nb, Si) Co-Doped TiO2 Ceramics
Author
Hicham Mahfoz Kotb 1   VIAFID ORCID Logo  ; Alshoaibi, Adil 2   VIAFID ORCID Logo  ; Mazher, Javed 2   VIAFID ORCID Logo  ; Shaalan, Nagih M 1   VIAFID ORCID Logo  ; Ahmad, Mohamad M 3   VIAFID ORCID Logo 

 Department of Physics, College of Science, King Faisal University, P.O. Box 400, Al-Ahsa 31982, Saudi Arabia; [email protected] (A.A.); [email protected] (J.M.); [email protected] (N.M.S.); [email protected] (M.M.A.); Physics Department, Faculty of Science, Assiut University, Assiut 71516, Egypt 
 Department of Physics, College of Science, King Faisal University, P.O. Box 400, Al-Ahsa 31982, Saudi Arabia; [email protected] (A.A.); [email protected] (J.M.); [email protected] (N.M.S.); [email protected] (M.M.A.) 
 Department of Physics, College of Science, King Faisal University, P.O. Box 400, Al-Ahsa 31982, Saudi Arabia; [email protected] (A.A.); [email protected] (J.M.); [email protected] (N.M.S.); [email protected] (M.M.A.); Department of Physics, Faculty of Science, The New Valley University, El-Kharga 72511, Egypt 
First page
4701
Publication year
2022
Publication date
2022
Publisher
MDPI AG
e-ISSN
19961944
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2686111940
Copyright
© 2022 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.