2015
DOI: 10.1021/acs.jpclett.5b02290
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Comparison of Recombination Dynamics in CH3NH3PbBr3 and CH3NH3PbI3 Perovskite Films: Influence of Exciton Binding Energy

Abstract: Understanding carrier recombination in semiconductors is a critical component when developing practical applications. Here we measure and compare the monomolecular, bimolecular, and trimolecular (Auger) recombination rate constants of CH3NH3PbBr3 and CH3NH3PbI3. The monomolecular and bimolecular recombination rate constants for both samples are limited by trap-assisted recombination. The bimolecular recombination rate constant for CH3NH3PbBr3 is ∼3.3 times larger than that for CH3NH3PbI3 and both are in line w… Show more

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Cited by 357 publications
(364 citation statements)
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“…[21] The excitonic contribution does not allow to directly evaluate the bandgap but requires a deconvolution of the excitonic versus bulk continuum contributions. [22] We followed the approach from Green and co-workers who simulated the spectrum near the band gap with the Elliott's equation in order to distinguish the excitonic versus the continuum contributions to the total absorption for iodide as well as bromide perovskites. [23] The exciton binding energy (R ex ) and band gap (E g ) are well fitted as 40.0 meV and 2.409 eV at 295 K from Figure S6 (Supporting Information), and these values are extremely close to the recent findings for CH 3 NH 3 PbBr 3 .…”
Section: Resultsmentioning
confidence: 99%
“…[21] The excitonic contribution does not allow to directly evaluate the bandgap but requires a deconvolution of the excitonic versus bulk continuum contributions. [22] We followed the approach from Green and co-workers who simulated the spectrum near the band gap with the Elliott's equation in order to distinguish the excitonic versus the continuum contributions to the total absorption for iodide as well as bromide perovskites. [23] The exciton binding energy (R ex ) and band gap (E g ) are well fitted as 40.0 meV and 2.409 eV at 295 K from Figure S6 (Supporting Information), and these values are extremely close to the recent findings for CH 3 NH 3 PbBr 3 .…”
Section: Resultsmentioning
confidence: 99%
“…Common Requirements [46,208] Copyright 2016, Nature Magneto-optical absorption spectroscopy [69] Polycrystalline 3D 22 Magneto-optical absorption spectroscopy [71] Polycrystalline 3D 2 Spectroscopic ellipsometry [66] Polycrystalline 3D 13 Optical absorption [72] Polycrystalline 3D 7 Electroabsorption Spectroscopy [8] Polycrystalline 3D 12 Magneto-optical absorption spectroscopy [73] CH3NH3PbBr3 Microcrystalline 3D 84 X-ray spectroscopy/Temperature dependent PL [74] Nanoparticle 3D 320 X-ray spectroscopy [74] Polycrystalline 3D 76 Magnetoabsorption [71] Polycrystalline 3D 40 Optical absorption [72] CH3NH3PbI3-xClx Polycrystalline 3D 55 Optical absorption [67] Polycrystalline 3D 10 Magneto-optical absorption spectroscopy [73] CH(NH2)2PbI3 Polycrystalline 3D 10 Magneto-optical absorption spectroscopy [73] CH(NH2)2PbBr3 Polycrystalline 3D 24 Magneto-optical absorption spectroscopy [73] (C9H19NH3)2PbI4 n/a 2D > 330 Temperature dependent PL [75] (C10H21NH3)2PbI4 Single crystal 2D 370 Optical absorption [76] (C6H5C2H4NH3)2PbI4 Polycrystalline 2D 350 Optical absorption [77] (NH2C(I)=NH2)3PbI5 n/a 1D > 410 Optical absorption [75] (CH3NH3)4PbI6•2H2O n/a 0D 545 Optical absorption [75] Eb: Exciton binding energy, PL: Photoluminescence Reproduced with permission. [98] Copyright 2014, Nature Publishing Group.…”
Section: Light Harvester Light Emittermentioning
confidence: 99%
“…The reduction of charge recombination in bulk film requires high quality perovskite film with full surface coverage [26][27][28], large crystal size [15,29,30] and low defect density [31][32][33]. The post-treatment using a strong Lewis base is a very effective method to improve the quality of lead halide perovskite films [34][35][36][37][38][39][40][41][42].…”
Section: Introductionmentioning
confidence: 99%