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Direct Measurement of the Exciton Binding Energy and Effective Masses for Charge carriers in Organic-Inorganic Trihalide Perovskites P. Plochocka Laboratoire National des Champs Magnétiques Intenses, CNRS-UJF-UPS-INSA, France Introduction Idea of perovskite solar cell: http://en.wikipedia.org/wiki/Perovskite_solar_cel What do we need from THE solar cell? 1. 2. 3. High optical absorption and quantum conversion efficiency Low carrier effective mass, long diffusion lengths Possibly low band gap low processing costs http://en.wikipedia.org/wiki/Perovskite_solar_cel S. D. Stranks et al., Science 342, 2013 What do we know? Saddle point nature of M Channel for holes M->R What do we know? Transition E1/2,g E1/2,u At R – 1st BG, ~1.6 eV At M – 2nd BG ~2.8 eV Secondary transitions at R – contribution to 2 BG What is the binding energy? There is a lot of controversy in literature about the value of the binding energy: 2-50meV Motivation What is the character of the photo created carriers in perovskite? Electron hole pair bound into exciton? What is the binding energy than? Other basic parameters of the system as for example mass…… How? Transmission measurements in high magnetic field Typical results Transmission of the white light through the sample of CH3NH3PbI3 at 4K: Minima observed in the spectra correspond to the absorption Differential spectra Analysis Energy of the absorption as a function of magnetic field: 2.2 Can we use a hydrogen model to fit the data? Energy (eV) 2.1 2.0 1.9 1.8 1.7 0 20 40 60 80 Magnetic Field (T) 100 120 140 Analysis Energy of the absorption as a function of magnetic field: We use theoretical model by Makado and McGill (numerical solution for the hydrogen atom in high magnetic field) 2.2 R* = 16 meV m* = 0.104 2.1 Energy (eV) R*=m*e4/2ћ2ε∞2 ε∞= 9 2.0 1.9 1.8 2s 1.7 1s 0 20 40 60 80 100 120 140 Magnetic Field (T) Makado, P.C. and McGill, N.C., Energy levels of a neutral hydrogen-like system in a 322 constant magnetic field of arbitary strength, J. Phys, C: Solid State Physics. 19 873 (1986) Analysis Free electron term: Energy of the absorption as a function of magnetic field: = + (N+1/2)ℏ ± 1/2 2.2 – cyclotron energy Zeeman energy Energy (eV) 2.1 2.0 1.9 1.8 2s 1.7 1s 0 20 40 60 80 Magnetic Field (T) 100 120 140 ff Discussion The observation of the 2s transition places strong constraints upon the exciton binding energy Slope and separation of the high field, high quantum number Landau levels strongly constrain the reduced effective mass value The excitonic transitions dominate for the N=0 landau level (1s, 2s) and the N=1 (1,0) level up to ~50T, and free electrons dominate for N=1 above 50T and for all higher Landau levels Temperature dependence High temperature data Single wavelength transmission vs magnetic field Broadband transmission vs magnetic field Landau fan chart Smaller binding energy at high temperature Who is working on it…… Magnetic field measurements: broadband transmission up to 70T Quantum electronics group D. K. Maude P. Plochocka Magnetic field measurements: single wavelength measurements up to 150T MegaGauss Olivier Portugall Oleksiy Drachenko Atsuhiko.Miyata (post doc) Zhou Yang phD A.A. Mitioglu phD R J NICHOLAS K. Galkowski phD Samuel D. Stranks Henry J. Snaith Jacob Tse-Wei Wang Clarendon Laboratory Parks Road Oxford OX1 3PU Perspectives……. We are currently working on….. CH3NH3PbI3-xClx CH(NH2)2PbI3 , CH(NH2)2PbBr3 Continuation of magnetic field measurements with circular polarization……. K. Galkowski working on spatial mapping as a function of temperature Time resolved measurements (pump probe and time resolved micro PL in ps range Semiconductor Nanowires, layer materials as dichalcogenides, graphene….. Combination of high/moderate magnetic field, low temp (mK), time resolved micro - spectroscopy Pulsed magnetic fields 14 MJ, 24 kV, 1 GW, 80 Tesla Transmission Single-turn coils 300 T in 5 mm diameter 150 T in 10 mm diameter 5 µs duration Repetitive experiments Huge dB/dt makes experiments difficult ‘Perovskite’ structure (CaTiO3) ABX3 (CH3NH3)PbI3 http://en.wikipedia.org/wiki/Perovskite_solar_cel http://en.wikipedia.org/wiki/Perovskite_solar_cel H.-S. Kim et al., Scientific Reports 2, 2012 • High optical absorption and quantum conversion efficiency • Low carrier effective mass, long diffusion lengths • Possibly low band gap • High optical absorption and quantum conversion efficiency • Low carrier effective mass, long diffusion lengths • Possibly low band gap + low processing costs hydrolysis Hydrolisis at ~1,7 eV Simplification of the system - due to higher bandgap, less perovskite SC than Si SC are to be connected in series J. Luo et al., Science 346 (2014) Solid: (CH3NH3)PbBr3 Dashed: (CH3NH3)PbI3 A. Kojima et al., J. Am. Chem. Soc 139 (2009) ISC VOC ISC PMAX VOC ISC PMAX VOC PMAX !! = VOC × ISC N. J. Jeon et al., Nature Materials 13, 2014 Michael D. McGehee, Nature Materials 13 2014 http://en.wikipedia.org/wiki/Perovskite_solar_cel The role of mesoporous sapphire scaffold in thin-layer solar cell – to reduce the number of defects during perovskite crystallization Ch. Wehrenfenning et al., Adv. Mater. 26, 2014 S. D. Stranks et al., Science 342, 2013 Ch. Wehrenfenning et al., Adv. Mater. 26, 2014 A.Amat et al., Nano Letters 14, 2014 BG: 1.73 eV A3 per unit vol: 222 ~1.6eV 248 ~1.5 eV 256 The role of symmetry and H-I bonds during substance crystallization Trigonal FA vs. tetragonal MA –enhanced Pb-I interaction in FA results in more “Pb” character of CB, thus higher splittings due to SOC –> lowering FA bangap J. Even et al., J. Phys. Chem. C 118, 2014 J. Even et al., J. Phys. Chem. C 118, 2014 J. Even et al., J. Phys. Chem. C 118, 2014 Transition E1/2,g E1/2,u At R – 1st BG, ~1.6 eV At M – 2nd BG ~2.8 eV Secondary transitions at R – contribution to 2 BG J. Even et al., J. Phys. Chem. C 118, 2014 Saddle point nature of M Channel for holes M->R J. Even et al., J. Phys. Chem. C 118, 2014 J. Even et al., J. Phys. Chem. C 118, 2014 Above phase transition temperature – rotations of organic cation contribute to lowfrequency ε Lattice vibrations contributing to high energy branch unaffected by phase transition M. Ibrahim Dar et al., Nano Letters, 2014 D.Giovanni et al., Nano Letters, 2014 Elliot-Yafet scattering mechanism S.N Habisreutinger et al., Nano Letters 14, 2014 Introduction H.-S. Kim et al., Scientific Reports 2, 2012