Controlled growth of large grains in CH3NH3PbI3 perovskite films mediated by an intermediate liquid phase without an antisolvent for efficient solar cells
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F20%3A00539178" target="_blank" >RIV/68378271:_____/20:00539178 - isvavai.cz</a>
Nalezeny alternativní kódy
RIV/68407700:21230/20:00348160 RIV/00216208:11320/20:10421689
Výsledek na webu
<a href="https://doi.org/10.1021/acsaem.0c02441" target="_blank" >https://doi.org/10.1021/acsaem.0c02441</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1021/acsaem.0c02441" target="_blank" >10.1021/acsaem.0c02441</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Controlled growth of large grains in CH3NH3PbI3 perovskite films mediated by an intermediate liquid phase without an antisolvent for efficient solar cells
Popis výsledku v původním jazyce
Large grains with uniform morphologies of the perovskite films are important for stable, high-performance perovskite solar cells. Herein, an effective strategy to control the growth of large grains in the CH3NH3PbI3 perovskite films is demonstrated by forming an intermediate CH3NH3PbI3·methylammonium chloride (MACl)·xCH3NH2 liquid phase induced by CH3NH2 gas treatment in combination with a MACl additive without an antisolvent. This intermediate liquid phase enables the well-controlled growth of large grains up to 3 μm, highly uniform morphology, and higher crystallinity in the final CH3NH3PbI3 perovskite films. The high-quality CH3NH3PbI3 film derived from the CH3NH3PbI3·MACl·xCH3NH2 phase leads to enhanced carrier lifetime and reduced charge-trap density and nonradiative recombination of the perovskite films. In addition, the defect healing and reduced grain boundaries also greatly improve the environmental stability in ambient air.n
Název v anglickém jazyce
Controlled growth of large grains in CH3NH3PbI3 perovskite films mediated by an intermediate liquid phase without an antisolvent for efficient solar cells
Popis výsledku anglicky
Large grains with uniform morphologies of the perovskite films are important for stable, high-performance perovskite solar cells. Herein, an effective strategy to control the growth of large grains in the CH3NH3PbI3 perovskite films is demonstrated by forming an intermediate CH3NH3PbI3·methylammonium chloride (MACl)·xCH3NH2 liquid phase induced by CH3NH2 gas treatment in combination with a MACl additive without an antisolvent. This intermediate liquid phase enables the well-controlled growth of large grains up to 3 μm, highly uniform morphology, and higher crystallinity in the final CH3NH3PbI3 perovskite films. The high-quality CH3NH3PbI3 film derived from the CH3NH3PbI3·MACl·xCH3NH2 phase leads to enhanced carrier lifetime and reduced charge-trap density and nonradiative recombination of the perovskite films. In addition, the defect healing and reduced grain boundaries also greatly improve the environmental stability in ambient air.n
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10302 - Condensed matter physics (including formerly solid state physics, supercond.)
Návaznosti výsledku
Projekt
<a href="/cs/project/EF15_003%2F0000464" target="_blank" >EF15_003/0000464: Centrum pokročilé fotovoltaiky</a><br>
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2020
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
ACS APPLIED ENERGY MATERIALS
ISSN
2574-0962
e-ISSN
—
Svazek periodika
3
Číslo periodika v rámci svazku
12
Stát vydavatele periodika
US - Spojené státy americké
Počet stran výsledku
10
Strana od-do
12484-12493
Kód UT WoS článku
000618839200104
EID výsledku v databázi Scopus
2-s2.0-85097844598