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dc.contributor.authorGroenhof, Gerrit
dc.contributor.authorCliment, Clàudia
dc.contributor.authorFeist, Johannes
dc.contributor.authorMorozov, Dmitry
dc.contributor.authorToppari, J. Jussi
dc.date.accessioned2019-09-02T05:34:41Z
dc.date.available2019-09-02T05:34:41Z
dc.date.issued2019
dc.identifier.citationGroenhof, G., Climent, C., Feist, J., Morozov, D., & Toppari, J. J. (2019). Tracking Polariton Relaxation with Multiscale Molecular Dynamics Simulations. <i>Journal of Physical Chemistry Letters</i>, <i>10</i>(18), 5476-5483. <a href="https://doi.org/10.1021/acs.jpclett.9b02192" target="_blank">https://doi.org/10.1021/acs.jpclett.9b02192</a>
dc.identifier.otherCONVID_32660949
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/65384
dc.description.abstractWhen photoactive molecules interact strongly with confined light modes in optical cavities, new hybrid light-matter states form. They are known as polaritons and correspond to coherent superpositions of excitations of the molecules and of the cavity photon. The polariton energies and thus potential energy surfaces are changed with respect to the bare molecules, such that polariton formation is considered a promising paradigm for controlling photochemical reactions. To effectively manipulate photochemistry with confined light, the molecules need to remain in the polaritonic state long enough for the reaction on the modified potential energy surface to take place. To understand what determines this lifetime, we have performed atomistic molecular dynamics simulations of room-temperature ensembles of rhodamine chromophores strongly coupled to a single confined light mode with a 15 fs lifetime. We investigated three popular experimental scenarios and followed the relaxation after optically pumping (i) the lower polariton, (ii) the upper polariton or (iii) uncoupled molecular states. The results of the simulations suggest that the lifetime of the optically accessibe lower and upper polaritons are limited by (i) ultra-fast photo-emission due to the low cavity lifetime and (ii) reversible population transfer into the 'dark' state manifold. Dark states are superpositions of molecular excitations but with much smaller contributions from the cavity photon, decreasing their emission rates and hence increasing their lifetimes. We find that population transfer between polaritonic modes and dark states is determined by the overlap between the polaritonic and molecular absorption spectra. Importantly, excitation can also be transferred "upwards" from the lower polariton into the dark-state reservoir due to the broad absorption spectra of the chromophores, contrary to the common conception of these processes as a "one-way" relaxation from the dark states down to the lower polariton. Our results thus suggest that polaritonic chemistry relying on modified dynamics taking place within the lower polariton manifold requires cavities with sufficiently long lifetimes and, at the same time, strong light-matter coupling strengths to prevent the back-transfer of excitation into the dark states.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherAmerican Chemical Society
dc.relation.ispartofseriesJournal of Physical Chemistry Letters
dc.rightsIn Copyright
dc.subject.otherpolaritons
dc.subject.othermolecular dynamics simulations
dc.titleTracking Polariton Relaxation with Multiscale Molecular Dynamics Simulations
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201909023989
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosKemian laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.laitosDepartment of Chemistryen
dc.contributor.oppiaineFysikaalinen kemiafi
dc.contributor.oppiainePhysical Chemistryen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.format.pagerange5476-5483
dc.relation.issn1948-7185
dc.relation.numberinseries18
dc.relation.volume10
dc.type.versionacceptedVersion
dc.rights.copyright© 2019 American Chemical Society
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber290677
dc.relation.grantnumber289947
dc.subject.ysovalokemia
dc.subject.ysomolekyylidynamiikka
dc.subject.ysopolaritonit
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p7201
jyx.subject.urihttp://www.yso.fi/onto/yso/p29332
jyx.subject.urihttp://www.yso.fi/onto/yso/p38894
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1021/acs.jpclett.9b02192
dc.relation.funderSuomen Akatemiafi
dc.relation.funderSuomen Akatemiafi
dc.relation.funderResearch Council of Finlanden
dc.relation.funderResearch Council of Finlanden
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundingprogramAcademy Project, AoFen
jyx.fundinginformationThis work was supported by the Academy of Finland (Grants 289947 to JJT; 290677 and to GG) as well as the European Research Council (ERC-2016-StG-714870 to JF) and the Spanish Ministry for Science, Innovation, and Universities - AEI (RTI2018-099737-B-I00 to JF).
dc.type.okmA1


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