1989
DOI: 10.1002/pssa.2211140263
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Temperature Dependence of the Mössbauer Spectra of CsSnCl3

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Cited by 5 publications
(5 citation statements)
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“…Figure shows the XRD patterns of the cubic MM-1 h-HT materials stored in inert atmosphere at different temperatures. The cubic structure was maintained after three months at 298 K, indicating that the as-prepared cubic CsSnCl 3 material possessed notably enhanced structural stability compared to the previously reported cubic CsSnCl 3 materials, which transformed to the white monoclinic CsSnCl 3 materials after 1 day. ,, One possible explanation may be related to the nanograins in the as-prepared cubic CsSnCl 3 material. It has been reported for many cubic perovskites that the small grains could increase the surface energy (surface to volume ratio) and thus stabilize the cubic structure. , Moreover, the lattice strain in the as-prepared cubic CsSnCl 3 material could induce a lattice distortion, which was also regarded as an effect that improved the stability of the cubic structure. Another reason for the enhancement in this structural stability was that the tin vacancy in the as-prepared cubic phase could not only produce a lattice distortion, but also create the locations with strengthened Cs–Cl bonds (Figure S3), thereby increasing the energy barrier for the octahedral titling of the cubic structure. , The as-prepared cubic phase can be kept at a lower temperature of 283 K for 1 day.…”
Section: Resultsmentioning
confidence: 73%
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“…Figure shows the XRD patterns of the cubic MM-1 h-HT materials stored in inert atmosphere at different temperatures. The cubic structure was maintained after three months at 298 K, indicating that the as-prepared cubic CsSnCl 3 material possessed notably enhanced structural stability compared to the previously reported cubic CsSnCl 3 materials, which transformed to the white monoclinic CsSnCl 3 materials after 1 day. ,, One possible explanation may be related to the nanograins in the as-prepared cubic CsSnCl 3 material. It has been reported for many cubic perovskites that the small grains could increase the surface energy (surface to volume ratio) and thus stabilize the cubic structure. , Moreover, the lattice strain in the as-prepared cubic CsSnCl 3 material could induce a lattice distortion, which was also regarded as an effect that improved the stability of the cubic structure. Another reason for the enhancement in this structural stability was that the tin vacancy in the as-prepared cubic phase could not only produce a lattice distortion, but also create the locations with strengthened Cs–Cl bonds (Figure S3), thereby increasing the energy barrier for the octahedral titling of the cubic structure. , The as-prepared cubic phase can be kept at a lower temperature of 283 K for 1 day.…”
Section: Resultsmentioning
confidence: 73%
“…The cubic structure was maintained after three months at 298 K, indicating that the as-prepared cubic CsSnCl 3 material possessed notably enhanced structural stability compared to the previously reported cubic CsSnCl 3 materials, which transformed to the white monoclinic CsSnCl 3 materials after 1 day. 27,37,38 One possible explanation may be related to the nanograins in the as-prepared cubic CsSnCl 3 material. It has been reported for many cubic perovskites that the small grains could increase the surface energy (surface to volume ratio) and thus stabilize the cubic structure.…”
Section: ■ Results and Discussionmentioning
confidence: 99%
“…The values of (6E/E + 3kT/2mc2) were found to decrease linearly with 1/T. With the temperature coefficient a set to zero and using the value of the slope of the (6E/E + 3kT/2mcZ) versus 1/T plot, the Debye temperature OD for CsSnBr, was estimated to be 260 K. A similar temperature dependence was observed for the (6E/E + 3kT/2mc2) values of CsSnC1, for which the Debye temperature was found to be 399 K [6].…”
mentioning
confidence: 52%
“…1 shows the variation of isomer shifts with temperature. These values, calculated relative to cl-tin, are typical of the trihalogenostannates [4,9]; an earlier Mossbauer work by'us revealed isomer shift values of around 1.60 mm/s for CsSnC1, [6]. For CsSnBr,, the isomer shift decreases linearly with temperature from 2.05 mm/s at 82 K to 1.91 mm/s at 280 K. However, at around 285 K, it increases on heating the absorber to 327 K. Scaife and co-workers [2] found that the lattice symmetry changes from a cubic perovskite, with a = 0.580 nm, to a tetragonally distorted perovskite, with a = 1.159 nm and c = 1.161 nm, at 292 K. In view of this, the anomaly observed in the temperature dependence of the isomer shift is indicative of a structural transformation at around 285 K.…”
mentioning
confidence: 94%
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