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dc.contributor.authorMandal, Bikramaditya
dc.contributor.authorPatkowski, Konrad
dc.contributor.authorGarcía Jambrina, Pablo 
dc.contributor.authorAoíz Moleres, Francisco Javier
dc.contributor.authorBalakrishnan, Naduvalath
dc.date.accessioned2025-05-09T08:17:52Z
dc.date.available2025-05-09T08:17:52Z
dc.date.issued2025
dc.identifier.citationBikramaditya Mandal, Konrad Patkowski, Pablo G. Jambrina, F. Javier Aoiz, Naduvalath Balakrishnan; Stereodynamics of cold HD and D2 collisions with He. J. Chem. Phys. 7 March 2025; 162 (10): 104201. https://doi.org/10.1063/5.0250522es_ES
dc.identifier.issn0021-9606
dc.identifier.urihttp://hdl.handle.net/10366/164973
dc.description.abstract[EN] We present a comprehensive quantum mechanical study of stereodynamic control of HD + He and D2 + He collisions that have been probed experimentally by Perreault et al. [J. Phys. Chem. Lett. 13, 10912 (2022)] using Stark-induced adiabatic Raman passage (SARP) techniques. Our calculations utilize a highly accurate full-dimensional H2 + He interaction potential with diagonal Born–Oppenheimer correction appropriate for HD and D2 isotopomers. The results show that rotational quenching of HD from j = 2 → j′ = 0 in v = 2, j = 2 → j′ = 1 in v = 2 and v = 4, and j = 4 → j′ = 3 in v = 4 is dominated by an l = 1 shape resonance located between 0.1 and 1.0 cm−1. For collision energies less than 0.1 cm−1, isotropic scattering prevails. An l = 1 resonance centered around 0.02 cm−1 is also found to dominate the j = 2 → j′ = 0 and j = 4 → j′ = 2 transitions in v = 4 for He–D2 collisions consistent with our prior studies of Δj = −2 transition in He + D2(v = 2, j = 2) collisions. Our analysis does not support the hypothesis of Perreault et al. [J. Phys. Chem. Lett. 13, 10912 (2022)] that a strong l = 2 resonance controls the angular distribution for Δj = −2 transition for both systems. Despite improvements in the development of the potential energy surface, a good agreement with SARP experiments for v = 2 is achieved only when contributions from collision energies less than 1.0 cm−1 were excluded in the computation of velocity averaged differential rate coefficients for both systems. This could be due to some uncertainties in the velocity spread in the experiment that employs co-propagation of the collision partners and possibly, the neglect of transverse velocities in the simulation of the experiment.es_ES
dc.format.mimetypeapplication/pdf
dc.language.isoenges_ES
dc.publisherAIP Publishinges_ES
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subjectQuantum chemistryes_ES
dc.subjectReaction dynamicses_ES
dc.subjectStereodynamicses_ES
dc.titleStereodynamics of cold HD and D2 collisions with Hees_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publishversionhttps://doi.org/10.1063/5.0250522es_ES
dc.identifier.doi10.1063/5.0250522
dc.relation.projectIDPID2023-147215NB-I00es_ES
dc.relation.projectIDPID2021- 122839NB-I00es_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.identifier.essn1089-7690
dc.journal.titleThe Journal of Chemical Physicses_ES
dc.volume.number162es_ES
dc.issue.number10es_ES
dc.page.initial104201es_ES
dc.type.hasVersioninfo:eu-repo/semantics/submittedVersiones_ES


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