<HashMap><database>biostudies-literature</database><scores/><additional><omics_type>Unknown</omics_type><volume>35(4)</volume><submitter>Monacelli L</submitter><pubmed_abstract>CsSnI&lt;sub>3&lt;/sub> is a promising ecofriendly solution for energy harvesting technologies. It exists at room temperature in either a black perovskite polymorph or a yellow 1D double-chain, which irreversibly deteriorates in the air. In this work, we unveil the relative thermodynamic stability between the two structures with a first-principles sampling of the CsSnI&lt;sub>3&lt;/sub> finite-temperature phase diagram, discovering how it is driven by anomalously large quantum and anharmonic ionic fluctuations. Thanks to a comprehensive treatment of anharmonicity, the simulations deliver a remarkable agreement with known experimental data for the transition temperatures of the orthorhombic, rhombohedral, and cubic perovskite structures and the thermal expansion coefficient. We disclose how the perovsk</pubmed_abstract><journal>Chemistry of materials : a publication of the American Chemical Society</journal><pagination>1702-1709</pagination><full_dataset_link>https://www.ebi.ac.uk/biostudies/studies/S-EPMC9979598</full_dataset_link><repository>biostudies-literature</repository><pubmed_title>First-Principles Thermodynamics of CsSnI&lt;sub>3&lt;/sub>.</pubmed_title><pmcid>PMC9979598</pmcid><pubmed_authors>Marzari N</pubmed_authors><pubmed_authors>Monacelli L</pubmed_authors></additional><is_claimable>false</is_claimable><name>First-Principles Thermodynamics of CsSnI&lt;sub>3&lt;/sub>.</name><description>CsSnI&lt;sub>3&lt;/sub> is a promising ecofriendly solution for energy harvesting technologies. It exists at room temperature in either a black perovskite polymorph or a yellow 1D double-chain, which irreversibly deteriorates in the air. In this work, we unveil the relative thermodynamic stability between the two structures with a first-principles sampling of the CsSnI&lt;sub>3&lt;/sub> finite-temperature phase diagram, discovering how it is driven by anomalously large quantum and anharmonic ionic fluctuations. Thanks to a comprehensive treatment of anharmonicity, the simulations deliver a remarkable agreement with known experimental data for the transition temperatures of the orthorhombic, rhombohedral, and cubic perovskite structures and the thermal expansion coefficient. We disclose how the perovsk</description><dates><release>2023-01-01T00:00:00Z</release><publication>2023 Feb</publication><modification>2025-05-29T16:30:18.973Z</modification><creation>2025-04-06T03:42:06.45Z</creation></dates><accession>S-EPMC9979598</accession><cross_references><pubmed>36873625</pubmed><doi>10.1021/acs.chemmater.2c03475</doi></cross_references></HashMap>