Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/4280
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dc.contributor.authorJayee, Bhumikaen_US
dc.contributor.authorMALPATHAK, SHREYASen_US
dc.contributor.authorMa, Xinyouen_US
dc.contributor.authorHase, William L.en_US
dc.date.accessioned2019-12-24T12:19:30Z
dc.date.available2019-12-24T12:19:30Z
dc.date.issued2019-11en_US
dc.identifier.citationJournal of Chemical Physics, 151(18).en_US
dc.identifier.issn0021-9606en_US
dc.identifier.issn1089-7690en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/4280-
dc.identifier.urihttps://doi.org/10.1063/1.5126805en_US
dc.description.abstractDirect dynamics simulations, using B3LYP/6-311++G(2d,2p) theory, were used to study the unimolecular and intramolecular dynamics of vibrationally excited CH3NC. Microcanonical ensembles of CH3NC, excited with 150, 120, and 100 kcal/mol of vibrational energy, isomerized to CH3CN nonexponentially, indicative of intrinsic non-Rice-Ramsperger-Kassel-Marcus (RRKM) dynamics. The distribution of surviving CH3NC molecules vs time, i.e., N(t)/N(0), was described by two separate functions, valid above and below a time limit, a single exponential for the former and a biexponential for the latter. The dynamics for the short-time component are consistent with a separable phase space model. The importance of this component decreases with vibrational energy and may be unimportant for energies relevant to experimental studies of CH3NC isomerization. Classical power spectra calculated for vibrationally excited CH3NC, at the experimental average energy of isomerizing molecules, show that the intramolecular dynamics of CH3NC are not chaotic and the C—N≡C and CH3 units are weakly coupled. The biexponential N(t)/N(0) at 100 kcal/mol is used as a model to study CH3NC → CH3CN isomerization with biexponential dynamics. The Hinshelwood-Lindemann rate constant kuni(ω,E) found from the biexponential N(t)/N(0) agrees with the Hinshelwood-Lindemann-RRKM kuni(ω,E) at the high and low pressure limits, but is lower at intermediate pressures. As found from previous work [S. Malpathak and W. L. Hase, J. Phys. Chem. A 123, 1923 (2019)], the two kuni(ω,E) curves may be brought into agreement by scaling ω in the Hinshelwood-Lindemann-RRKM kuni(ω,E) by a collisional energy transfer efficiency factor βc. The interplay between the value of βc, for the actual intermolecular energy transfer, and the ways the treatment of the rotational quantum number K and nonexponential unimolecular dynamics affect βc suggests that the ability to fit an experimental kuni(ω,T) with Hinshelwood-Lindemann-RRKM theory does not identify a unimolecular reactant as an intrinsic RRKM molecule.en_US
dc.language.isoenen_US
dc.publisherAIP Publishingen_US
dc.subjectVibrational-Energy-Transferen_US
dc.subjectChemical-Dynamics Simulationsen_US
dc.subjectSn2 Nucleophilic-Substitutionen_US
dc.subjectMethyl Isocyanideen_US
dc.subjectRate Constantsen_US
dc.subjectGateway Modesen_US
dc.subjectIntramolecular Dynamicsen_US
dc.subjectThermal-Isomerizationen_US
dc.subjectCD Overtonesen_US
dc.subjectMoleculesen_US
dc.subjectTOC-DEC-2019en_US
dc.subject2019en_US
dc.titleIs CH3NC isomerization an intrinsic non-RRKM unimolecular reactionen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Chemistryen_US
dc.identifier.sourcetitleJournal of Chemical Physicsen_US
dc.publication.originofpublisherForeignen_US
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