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dc.contributor.authorKhriachtchev Leonid
dc.contributor.authorLundell, Jan
dc.contributor.authorTapio, Salla
dc.contributor.authorDomanskaya, Alexandra V.
dc.contributor.authorRäsänen, Markku
dc.contributor.authorIsokoski, Karoliina
dc.date.accessioned2011-05-25T07:25:57Z
dc.date.available2011-05-25T07:25:57Z
dc.date.issued2011
dc.identifier.citationKhriachtchev, L., Lundell, J., Tapio, S., Domanskaya, A., Räsänen, M., & Isokoski, K. (2011). HXeOBr in a xenon matrix. <em>Journal of Chemical Physics</em>, 134 (12), 124307. <a href="http://dx.doi.org/10.1063/1.3570826">doi:10.1063/1.3570826</a>
dc.identifier.otherTUTKAID_45923
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/27070
dc.description.abstractWe report on a new noble-gas molecule HXeOBr prepared in a low-temperature xenon matrix from the HBr and N2O precursors by UV photolysis and thermal annealing. This molecule is assigned with the help of deuteration experiments and ab initio calculations including anharmonic methods. The H−Xe stretching frequency of HXeOBr is observed at 1634 cm−1 , which is larger by 56 cm−1 than the frequency of HXeOH identified previously. The experiments show a higher thermal stability of HXeOBr molecules in a xenon matrix compared to HXeOH.
dc.language.isoeng
dc.publisherAmerican Institute of Physics.
dc.relation.ispartofseriesJournal of Chemical Physics
dc.subject.otherjalokaasu
dc.subject.otherksenon
dc.subject.otherab initio
dc.subject.otheratomien liikkuvuus
dc.subject.otherspektroskopia
dc.titleHXeOBr in a xenon matrix
dc.typeArticle
dc.identifier.urnURN:NBN:fi:jyu-201804202265
dc.contributor.laitosKemian laitosfi
dc.contributor.laitosDepartment of Chemistryen
dc.contributor.oppiaineKemiafi
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2011-05-24T21:30:05Z
dc.type.coarjournal article
dc.description.reviewstatuspeerReviewed
dc.format.pagerange124307
dc.relation.issn0021-9606
dc.relation.numberinseries12
dc.relation.volume134
dc.type.versionpublishedVersion
dc.rights.copyright© 2011 American Institute of Physics.
dc.rights.accesslevelopenAccessfi
dc.relation.doi10.1063/1.3570826


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