4.8 Article

Ultralow Absorption Coefficient and Temperature Dependence of Radiative Recombination of CH3NH3Pbl3 Perovskite from Photoluminescence

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JOURNAL OF PHYSICAL CHEMISTRY LETTERS
卷 6, 期 5, 页码 767-772

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AMER CHEMICAL SOC
DOI: 10.1021/acs.jpclett.5b00044

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  1. Australian Government through the Australian Renewable Energy Agency (ARENA)
  2. Australian Research Council

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Spectrally resolved photoluminescence is used to measure the band-to-band absorption coefficient alpha(BB)((h) over bar omega) of organic-inorganic hybrid perovskite methylammonium lead iodide (CH3NH3PbI3) films from 675 to 1400 nm. Unlike other methods used to extract the absorption coefficient, photoluminescence is only affected by band-to-band absorption and is capable of detecting absorption events at very low energy levels. Absorption coefficients as low as 10(-1)4 cm(-1) are detected at room temperature for long wavelengths, which is 14 orders of magnitude lower than reported values at shorter wavelengths. The temperature dependence of alpha(BB)((h) over bar omega) is calculated from the photoluminescence spectra of CH3NH3PbI3 in the temperature range 80-360 K. Based on the temperature-dependent alpha(BB)((h) over bar omega), the product of the radiative recombination coefficient and square of the intrinsic carrier density, B(T) x n(i)(2), is also obtained.

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