2017
DOI: 10.1016/j.jpcs.2017.08.030
|View full text |Cite
|
Sign up to set email alerts
|

First-principles investigation on the structural, elastic and electronic properties and mechanism on the photocatalytic properties for SrNbO3 and Sr0.97NbO3

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
2

Citation Types

0
7
0

Year Published

2018
2018
2024
2024

Publication Types

Select...
7

Relationship

0
7

Authors

Journals

citations
Cited by 10 publications
(7 citation statements)
references
References 57 publications
0
7
0
Order By: Relevance
“…To accurately determine the intrinsic film lattice parameter, a ∥ and a ⊥ were found from the reciprocal space map around the asymmetric 1̅03 diffraction peaks of Sr x NbO 3 and LSAT. Assuming the calculated Poisson ratio of 0.31, an intrinsic film lattice parameter of 4.000 ± 0.005 Å was extracted for the three samples marked with the red stars in Figure b. The difference between this value and that of bulk samples , and other thin films , may be attributed to Sr vacancies due to preferential resputtering of Sr atoms caused by negative ions impinging on the growing film .…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…To accurately determine the intrinsic film lattice parameter, a ∥ and a ⊥ were found from the reciprocal space map around the asymmetric 1̅03 diffraction peaks of Sr x NbO 3 and LSAT. Assuming the calculated Poisson ratio of 0.31, an intrinsic film lattice parameter of 4.000 ± 0.005 Å was extracted for the three samples marked with the red stars in Figure b. The difference between this value and that of bulk samples , and other thin films , may be attributed to Sr vacancies due to preferential resputtering of Sr atoms caused by negative ions impinging on the growing film .…”
Section: Resultsmentioning
confidence: 99%
“…Assuming the calculated Poisson ratio of 0.31, 35 an intrinsic film lattice parameter of 4.000 ± 0.005 Å was extracted for the three samples marked with the red stars in Figure 2b. The difference between this value and that of bulk samples 24,35 and other thin films 20,30 may be attributed to Sr vacancies due to preferential resputtering of Sr atoms caused by negative ions impinging on the growing film. 36 By following Vegard's law and Sr x NbO 3 ceramic studies, 27,28 a Sr concentration of x = 0.8 was predicted for all films.…”
Section: Resultsmentioning
confidence: 99%
“…The mechanisms of the visible-light absorption and photocatalysis in SrNbO 3 have been actively discussed so far. In the early stage, interband electron transition from partially occupied conduction band to unoccupied band above the conduction band (CB → B 1 ) was suggested as the origin of the visible-light absorption. , After that, alternative mechanisms, such as band gap narrowing by Sr vacancy and plasmon excitation in the conduction band, have been proposed to describe the visible-light absorption. It has been argued that the photocatalytic activity originates from high electron mobility and hot electron transfer .…”
Section: Introductionmentioning
confidence: 99%
“…The observed c ‐axis of SNO//GSO, at this pressure, is close to the value expected due to epitaxial strain and assuming a Poisson ratio ν = 0.31. [ 3 ] In contrast the c (SNO//LSAT) value is smaller than expected, indicating that the film is partially relaxed due to their larger structural mismatch. Films grown at lower pressure display expanded c‐parameters (≈4.12 Å), as commonly observed in oxygen deficient films [ 13 ] or with cation off‐stoichiometry.…”
Section: Resultsmentioning
confidence: 88%
“…It was then proposed that the relevant absorption in the visible occurs between the CB and B 1 . [ 1,3,4 ]…”
Section: Introductionmentioning
confidence: 99%