Orbital change manipulation metal-insulator transition temperature in W-doped VO2

A series of epitaxial V 1− x W x O 2 (0 ≤ x ≤ 0.76%) nanocrystalline films on c -plane sapphire substrates have been successfully synthesized. Orbital structures of V 1− x W x O 2 films with monoclinic and rutile states have been investigated by ultraviolet-infrared spectroscopy combined with first...

Full description

Saved in:
Bibliographic Details
Published inPhysical chemistry chemical physics : PCCP Vol. 17; no. 17; pp. 11638 - 11646
Main Authors He, Xinfeng, Zeng, Yijie, Xu, Xiaofeng, Gu, Congcong, Chen, Fei, Wu, Binhe, Wang, Chunrui, Xing, Huaizhong, Chen, Xiaoshuang, Chu, Junhao
Format Journal Article
LanguageEnglish
Published England 07.05.2015
Online AccessGet full text

Cover

Loading…
More Information
Summary:A series of epitaxial V 1− x W x O 2 (0 ≤ x ≤ 0.76%) nanocrystalline films on c -plane sapphire substrates have been successfully synthesized. Orbital structures of V 1− x W x O 2 films with monoclinic and rutile states have been investigated by ultraviolet-infrared spectroscopy combined with first principles calculations. Experimental and calculated results show that the overlap of π* and d orbitals increases with increasing W doping content for the rutile state. Meanwhile, in the monoclinic state, the optical band gap decreases from 0.65 to 0.54 eV with increasing W doping concentration. Clear evidence is found that the V 1− x W x O 2 thin film phase transition temperature change comes from orbital structure variations. This shows that, with increasing W doping concentration, the decrease of rutile d orbital occupancy can reduce the strength of V-V interactions, which finally results in phase transition temperature decrease. The experimental results reveal that the d orbital is very important for the VO 2 phase transition process. Our findings open a possibility to tune VO 2 phase transition temperature through orbital engineering. Using ultraviolet-infrared spectroscopy and first principles calculations, it is revealed that changes in the orbital structure can regulate the W-doped VO 2 phase transition temperature.
Bibliography:ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:1463-9076
1463-9084
DOI:10.1039/c4cp04889j