| Literature DB >> 35424566 |
Mai Higuchi1, Mizuri Yaguchi1, Miru Yoshida-Hirahara1, Hitoshi Ogihara1, Hideki Kurokawa1.
Abstract
Perovskite-type oxides have impacted various research fields, including materials and energy science. Despite their vast potential in various applications, general and simple synthesis methods for nano-perovskites remain limited. Herein, various nano-perovskites were synthesized by a facile approach involving the use of nanocarbons. The calcination of the nanocarbon deposited with metal salts yielded nano-perovskites, emulating the morphology of nanocarbons. The accumulation of precursors (i.e., metal salts) on the surface of the nanocarbon during the evaporation of the solvent is the key step in which the precursors are homogeneously mixed prior to calcination. The homogeneity of the precursors facilitated low-temperature calcination that resulted in the formation of nano-perovskites. Various nano-perovskites, including LaMnO3, LaCoO3, LaFeO3, LaNiO3, LaAlO3, LaGaO3, CaMnO3, BaMnO3, SrMnO3, La0.7Sr0.3FeO3, La2CuO4, and Ca2Fe2O5, were successfully synthesized, demonstrating the simplicity and novelty of the method for the general synthesis of nano-perovskites. This journal is © The Royal Society of Chemistry.Entities:
Year: 2022 PMID: 35424566 PMCID: PMC8982278 DOI: 10.1039/d1ra08357k
Source DB: PubMed Journal: RSC Adv ISSN: 2046-2069 Impact factor: 3.361
Scheme 1Schematic diagram of the precursor accumulation (PA) method.
Fig. 1XRD patterns of perovskites prepared by the PA method using KB as the carbon source. The XRD patterns were indexed as LaMnO3, LaCoO3, LaFeO3, LaNiO3, LaAlO3, LaGaO3, La2CuO4, CaMnO3, Ca2Fe2O5, BaMnO3, SrMnO3, and La0.7Sr0.3FeO3 using JCPDS card no. 75-0440, 84-0848, 37-1493, 70-5757, 31-0022, 24-1102, 82-2142, 89-0666, 47-1744, 26-0168, 24-1213, and 89-1269, respectively.
Crystallite size and specific surface area of the perovskites prepared by the PA method using KB as the carbon source. Crystallite sizes were evaluated from XRD patterns using Scherrer's equation
| Perovskite | Crystallite size (nm) | Specific surface area (m2 g−1) |
|---|---|---|
| LaMnO3 | 13 | 44 |
| LaCoO3 | 24 | 24 |
| LaFeO3 | 20 | 36 |
| LaNiO3 | 16 | 7 |
| LaAlO3 | 29 | 24 |
| LaGaO3 | 35 | 4 |
| La2CuO4 | 48 | 4 |
| CaMnO3 | 37 | 5 |
| Ca2Fe2O5 | 35 | 32 |
| BaMnO3 | 37 | 9 |
| SrMnO3 | 28 | 10 |
| La0.7Sr0.3FeO3 | 15 | 33 |
Fig. 2SEM images of (a) KB, (b) SrMnO3, (c) LaMnO3, and (d) LaFeO3. Inset of (d): TEM image of LaFeO3. Carbon sources: KB (b and c), and CNFs (d).
Fig. 3STEM (a) and EDX elemental mapping images for (b) C, (c) La, and (d) Mn. The processes of nitrate deposition and calcination at 573 K were repeated 5 times prior to STEM/EDX analyses.
Fig. 4XRD patterns of the samples prepared by the deposition of (a–d) a mixture of lanthanum and manganese nitrates, (e) lanthanum nitrate, and (f) manganese nitrate on KB, following calcination at different temperatures.
Scheme 2Schematic diagram of precursor accumulation process on the carbon substrate.