2022
DOI: 10.1021/acs.jpclett.2c01463
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Phase-Stable and Highly Luminescent CsPbI3 Perovskite Nanocrystals with Suppressed Photoluminescence Blinking

Abstract: Despite their low band gap, the utility of CsPbI 3 nanocrystals (NCs) in solar photovoltaic and optoelectronic applications is rather limited because of their phase instability and photoluminescence (PL) intermittency. Herein we show that phase-pure, monodispersed, stable and highly luminescent CsPbI 3 NCs can be obtained by tweaking the conventional hot-injection method employing NH 4 I as an additional precursor. Single-particle studies show a significant suppression of PL blinking. Among all NCs studied, 60… Show more

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Cited by 18 publications
(40 citation statements)
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“…The past few years have witnessed the great promise of six-faceted ({110}, {002}) all-inorganic perovskite NCs (CsPbX 3 ; X = Br, Cl, I) in photovoltaic and optoelectronic applications. Their unique optical properties, such as near-unity photoluminescence quantum yields (PLQYs), narrow emission spectra, tunable photoluminescence (PL) in the visible region, long carrier diffusion length, etc., are keys to their massive success in several real applications such as displays, lasers, LEDs and solar cells. Despite the vast accomplishments, six-faceted cube NCs are not free from challenges; in fact, many of them are directly linked to the device’s performance. One such example is the rapid cooling (∼0.5–0.7 ps) of hot carriers (HCs) in cubic nanocrystals (NCs), a significant setback toward achieving a power conversion efficiency (PCE) of a theoretically predicted value (∼66%) or at least to a Shockley–Queisser limiting value (∼33%). , Extensive efforts have been put forward in slowing down the cooling in perovskite materials to a time scale slower than the time needed for the extractions of HCs. Such attempts proposed several phenomena, including acoustical–optical phonon upconversion, hot-phonon bottleneck, large-polaron formation, Auger heating, etc., were responsible for slow cooling in perovskite materials. , For instance, Fu et al and Wang et al have observed decelerated cooling in perovskite materials exploiting the Auger heating and synergetic effect of doped alkali cations (K + , Cs + , Rb + ) reducing the phonon bottleneck threshold.…”
mentioning
confidence: 99%
“…The past few years have witnessed the great promise of six-faceted ({110}, {002}) all-inorganic perovskite NCs (CsPbX 3 ; X = Br, Cl, I) in photovoltaic and optoelectronic applications. Their unique optical properties, such as near-unity photoluminescence quantum yields (PLQYs), narrow emission spectra, tunable photoluminescence (PL) in the visible region, long carrier diffusion length, etc., are keys to their massive success in several real applications such as displays, lasers, LEDs and solar cells. Despite the vast accomplishments, six-faceted cube NCs are not free from challenges; in fact, many of them are directly linked to the device’s performance. One such example is the rapid cooling (∼0.5–0.7 ps) of hot carriers (HCs) in cubic nanocrystals (NCs), a significant setback toward achieving a power conversion efficiency (PCE) of a theoretically predicted value (∼66%) or at least to a Shockley–Queisser limiting value (∼33%). , Extensive efforts have been put forward in slowing down the cooling in perovskite materials to a time scale slower than the time needed for the extractions of HCs. Such attempts proposed several phenomena, including acoustical–optical phonon upconversion, hot-phonon bottleneck, large-polaron formation, Auger heating, etc., were responsible for slow cooling in perovskite materials. , For instance, Fu et al and Wang et al have observed decelerated cooling in perovskite materials exploiting the Auger heating and synergetic effect of doped alkali cations (K + , Cs + , Rb + ) reducing the phonon bottleneck threshold.…”
mentioning
confidence: 99%
“…The peaks at 2854 and 2920 cm –1 are attributed to the stretching vibration of CH 2 and CH 3 in OA and OAm, respectively. The characteristic peak at 1465 cm –1 originates from the in-plane bending oscillation of OAm and OA ligands . However, the characteristic peaks at 1095 and 1260 cm –1 were only observed in SDBS-CsPbI 3 NCs, corresponding to S–O and SO, respectively .…”
Section: Resultsmentioning
confidence: 96%
“…Both samples were indexed as the and OA ligands. 31 However, the characteristic peaks at 1095 and 1260 cm −1 were only observed in SDBS-CsPbI 3 NCs, corresponding to S−O and S�O, respectively. 44 This result confirmed the presence of SDBS ligands on the surface of CsPbI 3 NCs.…”
Section: ■ Results and Discussionmentioning
confidence: 98%
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