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Publication:
Experimental Approach to the Study of Anharmonicity in the Infrared Spectrum of Pyrene from 14 to 723 K

cris.lastimport.scopus2025-07-05T17:04:50Z
cris.lastimport.wos2025-06-29T17:50:16Z
cris.virtual.departmentO.A. Cagliarien_US
cris.virtual.journalanceE093274en_US
cris.virtual.languageeng
cris.virtual.orcid0000-0003-0602-6669en_US
cris.virtualsource.departmentf6bb02cc-3784-4625-bffc-f3feb6028229
cris.virtualsource.journalance97ff594c-8171-44f6-af65-41bd757a4bfa
cris.virtualsource.orcidf6bb02cc-3784-4625-bffc-f3feb6028229
datacite.rightsopen.access
dc.contributor.authorChakraborty, Shubhadipen_US
dc.contributor.authorMULAS, Giacomoen_US
dc.contributor.authorDemyk, Karineen_US
dc.contributor.authorJoblin, Christineen_US
dc.date.accessioned2022-03-29T10:35:54Z
dc.date.available2022-03-29T10:35:54Z
dc.date.issued2019en_US
dc.description.abstractQuantifying the effect of anharmonicity on the infrared spectrum of large molecules such as polycyclic aromatic hydrocarbons (PAHs) at high temperature is the focus of a number of theoretical and experimental studies, many of them motivated by astrophysical applications. We recorded the infrared spectrum of pyrene C16H10 microcrystals embedded in a KBr pellet over a wide range of temperature (14 -723 K) and studied the evolution of band positions, widths and integrated intensities with temperature. We identified jumps for some of the spectral characteristics of some bands in the [423- 473]K range. These were attributed to a change of phase from crystal to molten in condensed pyrene, which appears to affect more strongly bands involving large CH motions. Empirical anharmonic factors that describe the evolution of band positions and widths with temperature were retrieved from both phases over an unprecedented temperature range. The derived values were found to be consistent with available gas-phase data. We provide recommended values for anharmonic factors and conclude about the interest of the methodology to provide data of interest for comparison with theoretical models and as inputs of models that simulate the infrared emission of astro-PAHs.en_US
dc.format.mediumSTAMPAen_US
dc.identifier.adsbibcode2019JPCA..123.4139Cen_US
dc.identifier.doi10.1021/acs.jpca.8b11016en_US
dc.identifier.issn1089-5639en_US
dc.identifier.urihttp://hdl.handle.net/20.500.12386/32008
dc.identifier.urlhttp://arxiv.org/abs/1904.02899v1en_US
dc.identifier.urlhttps://pubs.acs.org/doi/10.1021/acs.jpca.8b11016en_US
dc.language.isoenen_US
dc.relation.ispartofJOURNAL OF PHYSICAL CHEMISTRY. A, MOLECULES, SPECTROSCOPY, KINETICS, ENVIRONMENT, & GENERAL THEORYen_US
dc.subject.ssdFIS/05 - ASTRONOMIA E ASTROFISICAen_US
dc.titleExperimental Approach to the Study of Anharmonicity in the Infrared Spectrum of Pyrene from 14 to 723 Ken_US
dc.typeArticle
dspace.entity.typePublication
inaf.apcnoen_US
inaf.author.countryITAen_US
inaf.author.countryFRAen_US
inaf.author.internationalen_US
inaf.openaccess1 – prodotto con file in versione Open Access (allegare il file al passo  5-Carica)en_US
miur.type262 Articolo in rivista
miur.type.refereeREF_1en_US
oaire.citation.endPage4148en_US
oaire.citation.issue19en_US
oaire.citation.startPage4139en_US
oaire.citation.volume123en_US

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