Related Experiment Video
Updated: Jul 2, 2026

Fabrication of Schottky Diodes on Zn-polar BeMgZnO/ZnO Heterostructure Grown by Plasma-assisted Molecular Beam Epitaxy
Published on: October 23, 2018
Temperature-dependent recombination dynamics in BH/ZnBr2 Co-doped CsPbI3 thin films
Haichuan Mu1, Kai Sheng1, Ruibin Wang2
1School of Physics, East China University of Science and Technology, 130 Meilong Road, Shanghai 200237, P. R. China. hcmu@ecust.edu.cn.
None:
Temperature-dependent photoluminescence (PL), time-resolved photoluminescence (TRPL), and X-ray photoelectron spectroscopy (XPS) measurements were employed to investigate the recombination dynamics and defect evolution in BH/ZnBr2 co-doped CsPbI3 thin films. The results show that moderate co-doping effectively suppresses trap-assisted non-radiative recombination and improves the structural stability of the perovskite films. In particular, the optimally doped BH-Zn-23.0 sample exhibits a relatively low and weakly temperature-dependent monomolecular recombination rate constant (k1), together with reduced exciton binding energy and suppressed exciton-phonon coupling, indicating improved defect passivation and reduced lattice disorder. In contrast, excessive ZnBr2 incorporation leads to a pronounced increase in k1 with increasing temperature, suggesting the activation of deep-level defect-assisted recombination pathways. A clear change in the temperature dependence of k1 is observed near 140 K for the heavily doped sample, implying the existence of a critical doping threshold associated with defect activation and structural instability. Furthermore, the optimized co-doped films exhibit enhanced ambient phase stability, maintaining the black phase for extended storage in air. These results demonstrate that the carrier recombination behavior and environmental stability of BH/ZnBr2 co-doped CsPbI3 are strongly governed by the temperature-dependent evolution of defect states.
Related Concept Videos
Colors and Magnetism
When atoms or molecules absorb light at the proper frequency, their electrons are excited to higher-energy orbitals. For many main group atoms and molecules, the absorbed photons are in the ultraviolet range of the electromagnetic spectrum, which cannot be detected by the human eye. For coordination compounds, the energy difference between the d orbitals often allows photons in the visible range to be absorbed and emitted, which is seen as colors by the human eye.
Valence Bond Theory