Highly Selective Sensing of C2H6O, HCHO, and C3H6O Gases by Controlling SnO2 Nanoparticle Vacancies
Source abstract
Abstract
In this study, we prepared SnO2 containing various types of defects by changing the calcination atmosphere. Positron annihilation spectroscopy and electron-spin resonance show that oxygen vacancies (VO••) are the predominant species after calcination in air, while triple VSn′′′′VO••VSn′′′′ vacancy associates are predominant after calcination in helium. The sensing performance indicates that SnO2 nanoparticles calcined in air, helium, and oxygen exhibit excellent sensing performance for ethanol, formaldehyde, and acetone gases, respectively. On the basis of in situ IR spectroscopy, the sensitivity of SnO2 improves by reducing the objective gas to CO2. The relationship between the sensing selectivity and defect type was investigated. According to the results, the sensing mechanisms are discussed in terms of the selective effects of different defects based on combining band theory. The present study paves the way for the development of high-selectivity sensors.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Gas Sensing Nanomaterials and Sensors · ZnO doping and properties · Luminescence Properties of Advanced Materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Key Laboratory for Green Chemical Process of Ministry of Education and School of Chemistry and Environmental Engineering, Wuhan Institute of Technology, Xiongchu Avenue, Wuhan 430073, China
Funding
National Natural Science Foundation of China
References (39)
Show source-provided references
1. 10.1126/science.123987910.1126/science.1239879 ↗
2. 10.1021/ja808433d10.1021/ja808433d ↗
3. 10.1021/jacs.5b1021210.1021/jacs.5b10212 ↗
4. 10.1002/adfm.20160581710.1002/adfm.201605817 ↗
5. 10.1002/anie.20120990310.1002/anie.201209903 ↗
6. 10.1021/am401883510.1021/am4018835 ↗
7. 10.1021/acsami.6b0111610.1021/acsami.6b01116 ↗
8. 10.1021/ja402956f10.1021/ja402956f ↗
9. 10.1021/acs.jpcc.6b0897310.1021/acs.jpcc.6b08973 ↗
10. 10.1021/acs.analchem.6b0402310.1021/acs.analchem.6b04023 ↗
11. 10.1021/jp804916g10.1021/jp804916g ↗
12. 10.1021/jp201816d10.1021/jp201816d ↗
13. 10.1039/C7TA08117K10.1039/C7TA08117K ↗
14. 10.1021/jp407296f10.1021/jp407296f ↗
15. 10.1021/acs.analchem.5b0226710.1021/acs.analchem.5b02267 ↗
16. 10.1021/ja501866r10.1021/ja501866r ↗
17. 10.1021/jp307693y10.1021/jp307693y ↗
18. 10.1021/acs.chemmater.5b0485010.1021/acs.chemmater.5b04850 ↗
19. 10.1016/j.snb.2015.06.09910.1016/j.snb.2015.06.099 ↗
20. 10.1038/srep1012210.1038/srep10122 ↗
21. 10.1021/cm401895x10.1021/cm401895x ↗
22. 10.1016/j.apsusc.2016.10.05210.1016/j.apsusc.2016.10.052 ↗
23. 10.1126/science.120044810.1126/science.1200448 ↗
24. 10.1016/j.apcatb.2016.12.01810.1016/j.apcatb.2016.12.018 ↗
25. 10.1002/smll.20170135410.1002/smll.201701354 ↗
26. 10.1063/1.497891710.1063/1.4978917 ↗
27. 10.1016/S0022-3697(98)00269-810.1016/S0022-3697(98)00269-8 ↗
28. 10.1039/c2jm13610d10.1039/c2jm13610d ↗
29. 10.1103/PhysRevLett.88.09550110.1103/PhysRevLett.88.095501 ↗
30. 10.1021/ja907256x10.1021/ja907256x ↗
31. 10.1002/ange.20170233210.1002/ange.201702332 ↗
32. 10.1039/c1cc11887k10.1039/c1cc11887k ↗
33. 10.1016/S0961-9534(97)10038-110.1016/S0961-9534(97)10038-1 ↗
34. 10.1021/acsami.6b1352010.1021/acsami.6b13520 ↗
35. 10.1021/acsami.5b0584510.1021/acsami.5b05845 ↗
36. 10.1016/j.physb.2009.11.08610.1016/j.physb.2009.11.086 ↗
37. 10.1016/j.jallcom.2017.11.18510.1016/j.jallcom.2017.11.185 ↗
38. 10.1021/acs.iecr.6b0006010.1021/acs.iecr.6b00060 ↗
39. 10.1021/acsami.7b0546810.1021/acsami.7b05468 ↗