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The dynamics of the H+D₂O→OD+HD reaction at 2.5 eV: experiment and theory

dc.contributor.authorBrouard, M.
dc.contributor.authorBurak, I
dc.contributor.authorMinayev, D.
dc.contributor.authorO'Keeffe, P.
dc.contributor.authorVallance, C.
dc.contributor.authorAoiz, F. J.
dc.contributor.authorBañares, L.
dc.contributor.authorCastillo, J. F.
dc.contributor.authorZhang, Dong H.
dc.contributor.authorCollins, Michael A.
dc.date.accessioned2015-10-12T05:11:23Z
dc.date.available2015-10-12T05:11:23Z
dc.date.issued2003-01-15
dc.date.updated2015-12-12T08:28:03Z
dc.description.abstractThe title reaction has been studied both experimentally and computationally at a mean collision energy of 2.48 eV. OD quantum state populations, rotational alignment parameters, rovibrational quantum state-resolved center-of-mass angular scattering distributions and HD co-product internal energy release distributions have been determined, along with OD quantum state averaged energy disposals. The experiments employ pulsed laserphotolysis coupled with polarized Doppler-resolved laser induced fluorescence detection of the radical products. The OD angular scattering distributions show a preference for scattering in the forward direction, and are quite different from those observed previously at the lower collision energy of 1.4 eV. So too are the kinetic energy release distributions, which reveal that the HD co-products are born significantly more internally excited at 2.48 eV than at 1.4 eV. The HD internal energy distributions obtained from analysis of the Doppler resolved profiles are in reasonable accord with that derived from the direct HD population measurements performed by Zare and co-workers [J. Chem. Phys. 98, 4636 (1993)] at collision energies around 2.7 eV. The data are compared in detail with the results of new quasi-classical trajectory(QCT) calculations employing two alternative potential energy surfaces (PESs), as well as with the results from previous QCT studies of the title reaction by other workers. Refinements to the most recent of the PESs employed here, that developed using the iterative methods of Collins and Zhang and co-workers [J. Chem. Phys. 115, 174 (2001)], are also described. The theoretical results obtained using this refined PES agree very well with many of the experimental observables, and the surface appears to be a significant improvement on those previously developed. However, even with this new PES, the QCT calculations at 2.48 eV overestimate the internal excitation of the HD products.
dc.description.sponsorshipThe Oxford group thanks the Royal Society and the EPSRC for research grants. J.F.C. acknowledges support from the Spanish Ministry of Science and Technology through the program ‘‘Ramo´n y Cajal.’’ The Spanish work has been financed by DGES (Project PB98-0762-C03-01). We also gratefully acknowledge the EU (through project number HPRN-CT-1999-00007) for their support of a Research Training Network.en_AU
dc.identifier.issn0021-9606en_AU
dc.identifier.urihttp://hdl.handle.net/1885/15884
dc.publisherAmerican Institute of Physics (AIP)
dc.rightshttp://www.sherpa.ac.uk/romeo/issn/0021-9606..."Publishers version/PDF may be used on author's personal website, institutional website or institutional repository" from SHERPA/RoMEO site (as at 12/10/15). Copyright 2003 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. The following article appeared in The Journal of Chemical Physics and may be found at https://doi.org/10.1063/1.1528896
dc.sourceThe Journal of Chemical Physics
dc.subjectKeywords: Atomic physics; Deuterium compounds; Electron scattering; Fluorescence; Ground state; Hydrogen; Iterative methods; Molecular vibrations; Monte Carlo methods; Photolysis; Pulsed laser applications; Quantum theory; Kinetic energy release distribution; Laser
dc.titleThe dynamics of the H+D₂O→OD+HD reaction at 2.5 eV: experiment and theory
dc.typeJournal article
local.bibliographicCitation.issue3en_AU
local.bibliographicCitation.lastpage1174en_AU
local.bibliographicCitation.startpage1162en_AU
local.contributor.affiliationBrouard, M, University of Oxford, United Kingdomen_AU
local.contributor.affiliationBurak, I, University of Oxford, United Kingdomen_AU
local.contributor.affiliationMinayev, D, University of Oxford, United Kingdomen_AU
local.contributor.affiliationO'Keeffe, P, University of Oxford, United Kingdomen_AU
local.contributor.affiliationVallance, C, University of Oxford, United Kingdomen_AU
local.contributor.affiliationAoiz, F, Universidad Complutense de Madrid, Spainen_AU
local.contributor.affiliationBanares, L, Universidad Complutense de Madrid, Spainen_AU
local.contributor.affiliationCastiglione, J, University of Florida, United States of Americaen_AU
local.contributor.affiliationZhang, Dong Hui, National University of Singapore, Singaporeen_AU
local.contributor.affiliationCollins, Michael, College of Physical and Mathematical Sciences, CPMS Research School of Chemistry, RSC General, The Australian National Universityen_AU
local.contributor.authoruidu7801246en_AU
local.description.notesImported from ARIESen_AU
local.description.refereedYes
local.identifier.absfor030703en_AU
local.identifier.ariespublicationMigratedxPub17014en_AU
local.identifier.citationvolume118en_AU
local.identifier.doi10.1063/1.1528896en_AU
local.identifier.scopusID2-s2.0-0037439716
local.publisher.urlhttps://www.aip.org/en_AU
local.type.statusPublished Versionen_AU

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