TY - JOUR
T1 - Dynamic Disorder, Band Gap Widening, and Persistent Near-IR Photoluminescence up to at Least 523 K in ASnI3 Perovskites (A = Cs+, CH3NH3 + and NH2-CHNH2 +)
AU - Kontos, Athanassios G.
AU - Kaltzoglou, Andreas
AU - Arfanis, Michalis K.
AU - McCall, Kyle M.
AU - Stoumpos, Constantinos C.
AU - Wessels, Bruce W
AU - Falaras, Polycarpos
AU - Kanatzidis, Mercouri
N1 - Funding Information:
This work was also supported by the Department of Energy, Office of Science, Basic Energy Sciences under Grant SC0012541 (synthesis and characterization of materials diffraction studies, interpretation of data M.G.K.). Use of the Advanced Photon Source at Argonne National Laboratory was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357.
Publisher Copyright:
© 2018 American Chemical Society.
PY - 2018/11/21
Y1 - 2018/11/21
N2 - We report temperature-dependent photoluminescence (PL) in polycrystalline ASnI3 perovskites (A = Cs+, CH3NH3 +, and HC(NH2)2 +), demonstrating extremely robust emission up to very high temperatures (523 K for CsSnI3). The PL peak energy (EPL) monotonically blueshifts with increasing temperature, indicating band gap widening. Variable temperature synchrotron powder X-ray diffraction analysis confirms that these changes are associated with progressive emphanitic off-centering and dynamic fluctuations of the perovskite lattice. In CsSnI3, three different temperature gradients of EPL are defined (0.29 meV K-1 below 200 K, 0.17 meV K-1 from 200 to 400 K, and 0.48 meV K-1 above 400 K), commensurate with the onset of dynamic structural disorder at 200 K and its saturation at 400 K as the Cs+ atoms rattle independently of the [SnI3]- perovskite lattice. These results explain how solution-processed perovskites with massive defect concentrations can yield high optoelectronic performance at elevated temperatures.
AB - We report temperature-dependent photoluminescence (PL) in polycrystalline ASnI3 perovskites (A = Cs+, CH3NH3 +, and HC(NH2)2 +), demonstrating extremely robust emission up to very high temperatures (523 K for CsSnI3). The PL peak energy (EPL) monotonically blueshifts with increasing temperature, indicating band gap widening. Variable temperature synchrotron powder X-ray diffraction analysis confirms that these changes are associated with progressive emphanitic off-centering and dynamic fluctuations of the perovskite lattice. In CsSnI3, three different temperature gradients of EPL are defined (0.29 meV K-1 below 200 K, 0.17 meV K-1 from 200 to 400 K, and 0.48 meV K-1 above 400 K), commensurate with the onset of dynamic structural disorder at 200 K and its saturation at 400 K as the Cs+ atoms rattle independently of the [SnI3]- perovskite lattice. These results explain how solution-processed perovskites with massive defect concentrations can yield high optoelectronic performance at elevated temperatures.
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U2 - 10.1021/acs.jpcc.8b10218
DO - 10.1021/acs.jpcc.8b10218
M3 - Article
AN - SCOPUS:85057165316
SN - 1932-7447
VL - 122
SP - 26353
EP - 26361
JO - Journal of Physical Chemistry C
JF - Journal of Physical Chemistry C
IS - 46
ER -