<HashMap><database>biostudies-literature</database><scores/><additional><submitter>Kim TJ</submitter><funding>Korean government</funding><funding>National Research Foundation</funding><pagination>e2207653</pagination><full_dataset_link>https://www.ebi.ac.uk/biostudies/studies/S-EPMC10190583</full_dataset_link><repository>biostudies-literature</repository><omics_type>Unknown</omics_type><volume>10(14)</volume><pubmed_abstract>Interlayer excitons (IXs) at the interface of heterostructures (HSs) with a staggered band alignment are fascinating quantum quasi-particles with light-emitting and long-lifetime characteristics. In this study, the energy band alignments (EBAs) of the HS of MAPbI&lt;sub>3&lt;/sub> perovskite thin sheets with CdSe-ZnS core-shell quantum dot (QD) layers are modulated by using different diameters of the QDs. Far-red IX emission is observed at 1.42 eV from the HS of MAPbI&lt;sub>3&lt;/sub> /CdSe-ZnS-QD (λ&lt;sub>em&lt;/sub>  = 645 nm) with type-II EBA owing to charge transfer. The lifetime of the far-red IXs is estimated to be 5.68 µs, which is considerably longer than that (0.715 ns) of the intralayer excitons from CdSe-ZnS-QD. With increasing incident excitation power, the PL peak and its intensity of IXs are blue-shifted and linearly increased, respectively, indicating a strong dipole alignment of far-red IXs at the heterojunction. Back focal plane imaging suggests that the directions of dipole moments of the IXs are relatively out-of-plane compared to those of the intralayer excitons (MAPbI&lt;sub>3&lt;/sub> and CdSe-ZnS-QD). Notably, the abnormal behavior of the optical characteristics is observed near the phase transition temperature (90 K) of MAPbI&lt;sub>3&lt;/sub> . MAPbI&lt;sub>3&lt;/sub> /CdSe-ZnS-QD HS photodetectors show the increase in photocurrent and detectivity compared to MAPbI&lt;sub>3&lt;/sub> at IX excitation.</pubmed_abstract><journal>Advanced science (Weinheim, Baden-Wurttemberg, Germany)</journal><pubmed_title>Far-Red Interlayer Excitons of Perovskite/Quantum-Dot Heterostructures.</pubmed_title><pmcid>PMC10190583</pmcid><funding_grant_id>2022R1A2C2009412</funding_grant_id><funding_grant_id>2021R1A2C2005885</funding_grant_id><pubmed_authors>Seo C</pubmed_authors><pubmed_authors>Kim TJ</pubmed_authors><pubmed_authors>Joo J</pubmed_authors><pubmed_authors>Lee SH</pubmed_authors><pubmed_authors>Kim J</pubmed_authors><pubmed_authors>Lee E</pubmed_authors></additional><is_claimable>false</is_claimable><name>Far-Red Interlayer Excitons of Perovskite/Quantum-Dot Heterostructures.</name><description>Interlayer excitons (IXs) at the interface of heterostructures (HSs) with a staggered band alignment are fascinating quantum quasi-particles with light-emitting and long-lifetime characteristics. In this study, the energy band alignments (EBAs) of the HS of MAPbI&lt;sub>3&lt;/sub> perovskite thin sheets with CdSe-ZnS core-shell quantum dot (QD) layers are modulated by using different diameters of the QDs. Far-red IX emission is observed at 1.42 eV from the HS of MAPbI&lt;sub>3&lt;/sub> /CdSe-ZnS-QD (λ&lt;sub>em&lt;/sub>  = 645 nm) with type-II EBA owing to charge transfer. The lifetime of the far-red IXs is estimated to be 5.68 µs, which is considerably longer than that (0.715 ns) of the intralayer excitons from CdSe-ZnS-QD. With increasing incident excitation power, the PL peak and its intensity of IXs are blue-shifted and linearly increased, respectively, indicating a strong dipole alignment of far-red IXs at the heterojunction. Back focal plane imaging suggests that the directions of dipole moments of the IXs are relatively out-of-plane compared to those of the intralayer excitons (MAPbI&lt;sub>3&lt;/sub> and CdSe-ZnS-QD). Notably, the abnormal behavior of the optical characteristics is observed near the phase transition temperature (90 K) of MAPbI&lt;sub>3&lt;/sub> . MAPbI&lt;sub>3&lt;/sub> /CdSe-ZnS-QD HS photodetectors show the increase in photocurrent and detectivity compared to MAPbI&lt;sub>3&lt;/sub> at IX excitation.</description><dates><release>2023-01-01T00:00:00Z</release><publication>2023 May</publication><modification>2025-04-25T22:28:13.921Z</modification><creation>2025-04-06T09:06:13.848Z</creation></dates><accession>S-EPMC10190583</accession><cross_references><pubmed>36938849</pubmed><doi>10.1002/advs.202207653</doi></cross_references></HashMap>