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Slow Cooling of Hot Polarons in Halide Perovskite Solar Cells.


ABSTRACT: Halide perovskites show unusual thermalization kinetics for above-bandgap photoexcitation. We explain this as a consequence of excess energy being deposited into discrete large polaron states. The crossover between low-fluence and high-fluence "phonon bottleneck" cooling is due to a Mott transition where the polarons overlap (n ? 1018 cm-3) and the phonon subpopulations are shared. We calculate the initial rate of cooling (thermalization) from the scattering time in the Fröhlich polaron model to be 78 meV ps-1 for CH3NH3PbI3. This rapid initial thermalization involves heat transfer into optical phonon modes coupled by a polar dielectric interaction. Further cooling to equilibrium over hundreds of picoseconds is limited by the ultralow thermal conductivity of the perovskite lattice.

SUBMITTER: Frost JM 

PROVIDER: S-EPMC5727468 | biostudies-literature | 2017 Dec

REPOSITORIES: biostudies-literature

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Slow Cooling of Hot Polarons in Halide Perovskite Solar Cells.

Frost Jarvist Moore JM   Whalley Lucy D LD   Walsh Aron A  

ACS energy letters 20171023 12


Halide perovskites show unusual thermalization kinetics for above-bandgap photoexcitation. We explain this as a consequence of excess energy being deposited into discrete large polaron states. The crossover between low-fluence and high-fluence "phonon bottleneck" cooling is due to a Mott transition where the polarons overlap (<i>n</i> ≥ 10<sup>18</sup> cm<sup>-3</sup>) and the phonon subpopulations are shared. We calculate the initial rate of cooling (thermalization) from the scattering time in  ...[more]

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