<HashMap><database>biostudies-literature</database><scores/><additional><submitter>Jin S</submitter><funding>Austrian Science Fund FWF</funding><funding>Ministerio de Ciencia, Innovaci?n y Universidades</funding><funding>Universidad de Valladolid</funding><pagination>3455-3465</pagination><full_dataset_link>https://www.ebi.ac.uk/biostudies/studies/S-EPMC12010328</full_dataset_link><repository>biostudies-literature</repository><omics_type>Unknown</omics_type><volume>129(15)</volume><pubmed_abstract>Although iron is the most abundant transition metal in the interstellar medium, its interaction with hydrogen─by far the most abundant element─in small gas-phase molecules or complexes is poorly understood. Herein, we study the infrared spectroscopy of cationic iron complexes with one and two dihydrogen ligands, Fe&lt;sup>+&lt;/sup>(H&lt;sub>2&lt;/sub>)&lt;sub>1,2&lt;/sub>, as well as their deuterated counterparts, Fe&lt;sup>+&lt;/sup>(D&lt;sub>2&lt;/sub>)&lt;sub>1,2&lt;/sub>, using infrared multiple photon dissociation (IRMPD) spectroscopy. Quantum chemical calculations, including multireference configuration interaction (MRCI) with spin-orbit coupling, are used to simulate the electronic and vibrational contributions to the spectra. Broad electronic transitions are observed in the studied energy range of 2230-4000 cm&lt;sup>-</pubmed_abstract><journal>The journal of physical chemistry. A</journal><pubmed_title>Infrared Multiple Photon Dissociation Spectroscopy of the H-H Stretching Mode and Low-Lying Electronic Transitions in Fe&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;sub&amp;gt;1,2&amp;lt;/sub&amp;gt; and Fe&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;(D&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;sub&amp;gt;1,2&amp;lt;/sub&amp;gt;.</pubmed_title><pmcid>PMC12010328</pmcid><funding_grant_id>10.55776/W1259</funding_grant_id><funding_grant_id>10.55776/P35013</funding_grant_id><funding_grant_id>CONREC-2021-265</funding_grant_id><pubmed_authors>Juanes M</pubmed_authors><pubmed_authors>Jin S</pubmed_authors><pubmed_authors>van der Linde C</pubmed_authors><pubmed_authors>Oncak M</pubmed_authors><pubmed_authors>Beyer MK</pubmed_authors></additional><is_claimable>false</is_claimable><name>Infrared Multiple Photon Dissociation Spectroscopy of the H-H Stretching Mode and Low-Lying Electronic Transitions in Fe&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;sub&amp;gt;1,2&amp;lt;/sub&amp;gt; and Fe&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;(D&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;sub&amp;gt;1,2&amp;lt;/sub&amp;gt;.</name><description>Although iron is the most abundant transition metal in the interstellar medium, its interaction with hydrogen─by far the most abundant element─in small gas-phase molecules or complexes is poorly understood. Herein, we study the infrared spectroscopy of cationic iron complexes with one and two dihydrogen ligands, Fe&lt;sup>+&lt;/sup>(H&lt;sub>2&lt;/sub>)&lt;sub>1,2&lt;/sub>, as well as their deuterated counterparts, Fe&lt;sup>+&lt;/sup>(D&lt;sub>2&lt;/sub>)&lt;sub>1,2&lt;/sub>, using infrared multiple photon dissociation (IRMPD) spectroscopy. Quantum chemical calculations, including multireference configuration interaction (MRCI) with spin-orbit coupling, are used to simulate the electronic and vibrational contributions to the spectra. Broad electronic transitions are observed in the studied energy range of 2230-4000 cm&lt;sup>-</description><dates><release>2025-01-01T00:00:00Z</release><publication>2025 Apr</publication><modification>2025-07-07T03:10:04.214Z</modification><creation>2025-07-07T03:10:04.214Z</creation></dates><accession>S-EPMC12010328</accession><cross_references><pubmed>40173356</pubmed><doi>10.1021/acs.jpca.5c00196</doi></cross_references></HashMap>