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Halogen–NH2 + Interaction, Temperature-Induced Phase Transition, and Ordering in (NH2CHNH2)PbX3 (X = Cl, Br, I) Hybrid Perovskites

Hybrid organic–inorganic FAPbX3 perovskites (FA = NH2CHNH2 +, X = Cl–, Br–, I–) are currently intensively investigated in solar cells. In this study, off-resonance Raman and far-IR absorption spectra of all single-halogen FAPbX3, as well as of mixed-halogen FAPbBr2X derivatives, are reported and ana...

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Bibliographic Details
Published in:Journal of physical chemistry. C 2020-04, Vol.124 (16), p.8479-8487
Main Authors: Kontos, Athanassios G, Manolis, Georgios K, Kaltzoglou, Andreas, Palles, Dimitrios, Kamitsos, Efstratios I, Kanatzidis, Mercouri G, Falaras, Polycarpos
Format: Article
Language:English
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Summary:Hybrid organic–inorganic FAPbX3 perovskites (FA = NH2CHNH2 +, X = Cl–, Br–, I–) are currently intensively investigated in solar cells. In this study, off-resonance Raman and far-IR absorption spectra of all single-halogen FAPbX3, as well as of mixed-halogen FAPbBr2X derivatives, are reported and analyzed. Vibrations of the PbX6 octahedra and librations of the FA cation lay at frequencies below 250 cm–1, while external and internal FA bands are identified above 200 cm–1. An increase in the frequencies of most vibrational bands is observed upon substituting lighter and more electronegative halides for heavier ones due to strengthening of the electrostatic interaction between X– and the FA NH2 + groups. Variable-temperature Raman measurements are also carried out for FAPbBr3 and FAPbCl3 in the 77–400 K range. Upon cooling, the three Pb–X Raman vibrations of the cubic structure, split into eight separate bands, signaling the transformation to the tetragonal phase at ∼240 K and ∼200 K for FAPbBr3 and FAPbCl3, respectively. At even lower temperatures, a successive phase transformation to low symmetry orthorhombic phases is evidenced. These temperature-induced effects are accompanied by intense narrowing, soft-mode behavior, and/or sudden frequency shift of specific Raman bands, attributed to ordering of the FA cation.
ISSN:1932-7447
1932-7455
DOI:10.1021/acs.jpcc.9b11334