2018
DOI: 10.1016/j.jechem.2018.01.006
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Ultrafast selective extraction of hot holes from cesium lead iodide perovskite films

Abstract: International audienc

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Cited by 23 publications
(25 citation statements)
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“…For <N 0 > ≈0.1, the η hot for EDT-NCs/Bphen is ≈72%. More recently, HC-extraction evidenced using the TA approach was also reported for a CsPbI 3 film with P3HT as the extraction layer by Shen et al [38] The near instantaneous disappearance of the hot-energy tail (within ≈0.3 ps) and the reduction of HC temperatures in CsPbI 3 /P3HT bilayers validate the efficient and extremely fast hot-hole injection into P3HT (Figure 10e). Comparatively, due to the faster HC cooling, the η hot of its bulk-film counterpart is approximately five times lower under similar photoexcitation conditions.…”
Section: Efficient Hc Extractionsupporting
confidence: 72%
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“…For <N 0 > ≈0.1, the η hot for EDT-NCs/Bphen is ≈72%. More recently, HC-extraction evidenced using the TA approach was also reported for a CsPbI 3 film with P3HT as the extraction layer by Shen et al [38] The near instantaneous disappearance of the hot-energy tail (within ≈0.3 ps) and the reduction of HC temperatures in CsPbI 3 /P3HT bilayers validate the efficient and extremely fast hot-hole injection into P3HT (Figure 10e). Comparatively, due to the faster HC cooling, the η hot of its bulk-film counterpart is approximately five times lower under similar photoexcitation conditions.…”
Section: Efficient Hc Extractionsupporting
confidence: 72%
“…Lastly, the cooled carriers will recombine (usually in nanosecond timescale -process 6). [22,[28][29][30][31][37][38][39][40][41][42][43][44][45] These studies include the 3) carrier-optical phonon interactions; 4) decay of optical phonons into acoustic phonons; 5) further phonon emission to thermal equilibrium; (6) onset of carrier recombination. Next, we trace the milestones of slow HC cooling phenomena in halide perovskites.…”
Section: Typical Hc Cooling Dynamicsmentioning
confidence: 99%
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“…Such hot carriers have higher carrier temperature, T C , than the crystal lattice, which dissipates in a very short period of time (hundreds of fs) through a phonon emission process. The T C can be calculated by fitting the TA spectra (the fitting curves are provided in the Supporting Information, see Figure S6) above the band edge (between 1.7 and 2 eV) to a Boltzmann distribution9a,b,11,12ΔA[]EeEEf/kBTcwhere, E f is the quasi‐Fermi energy and k B is the Boltzmann constant. Figure d shows the T c of MAPbI 3 film drops from ≈1500 to 600 K within ≈2 ps after photoexcitation, implying that the excess energy of the carriers was released to the crystal lattice through nonradiative pathways.…”
Section: Resultsmentioning
confidence: 99%
“…With a few studies uncovering qualitatively different cooling behavior exhibited by perovskites in comparison to other conventional semiconductor materials used in solar cells . However, the extraction of these hot carriers before they quickly relax to the band edges still remains largely elusive for the MAPbI 3 perovskite films; although there are few works about the extraction from other perovskites systems, including MAPbBr 3 , CsPbI 3 , and CsPbBr 3 perovskite nanocrystals.…”
Section: Introductionmentioning
confidence: 99%