Mostrar el registro sencillo del ítem

dc.contributor.authorRedondo Cristóbal, María del Pilar 
dc.contributor.authorSanz Novo, Miguel 
dc.contributor.authorLargo Cabrerizo, Antonio 
dc.contributor.authorBarrientos Benito, María Carmen 
dc.date.accessioned2020-10-07T08:07:48Z
dc.date.available2020-10-07T08:07:48Z
dc.date.issued2020
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Volume 492, Issue 2, 2020, Pages 1827–1833es
dc.identifier.issn0035-8711es
dc.identifier.urihttp://uvadoc.uva.es/handle/10324/42797
dc.descriptionProducción Científicaes
dc.description.abstractWe present a computational study of the different conformers of amino acetaldehyde. This molecule is a precursor of glycine and also an isomer of the detected molecules acetaldehyde and methylformamide. In addition, a previous theoretical result shows that amino acetaldehyde could be formed from the gas phase reaction of formamide with CH+5⁠. Different computational approaches, going from density functional theory (DFT) to coupled cluster (CC) calculations, are employed for the characterization of the amino acetaldehyde conformers. We locate four low-lying conformation on the singlet potential energy surface (PES), two with a synperiplanar arrangement of the carboxylic oxygen atom and the NH2 group, and the other two conformers with an anticlinal disposition. All levels of theory predict the conformer with a synperiplanar arrangement and the H atoms of the NH2 group pointing in the direction of the oxygen, denoted as in-sp-amino acetaldehyde, as the most stable. The viability of the interconversion processes between the four conformers in space is analysed. Relevant spectroscopic parameters to rotational spectroscopy with ‘spectroscopic’ accuracy at the composite level are reported. Vibrational frequencies and infrared intensities are also computed at the CC with single and double excitations (CCSD) level including anharmonic corrections. This information could help in the experimental characterization of amino acetaldehyde that could be considered as a good candidate molecule to be searched for in space.es
dc.format.mimetypeapplication/pdfes
dc.language.isoenges
dc.publisherRoyal Astronomical Societyes
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subject.classificationAstrobiologíaes
dc.subject.classificationAstroquímicaes
dc.titleAmino acetaldehyde conformers: structure and spectroscopic propertieses
dc.typeinfo:eu-repo/semantics/articlees
dc.rights.holder© 2019 The Authorses
dc.identifier.doi10.1093/mnras/stz3561es
dc.relation.publisherversionhttps://academic.oup.com/mnras/article-abstract/492/2/1827/5681404es
dc.identifier.publicationfirstpage1827es
dc.identifier.publicationissue2es
dc.identifier.publicationlastpage1833es
dc.identifier.publicationtitleMonthly Notices of the Royal Astronomical Societyes
dc.identifier.publicationvolume492es
dc.peerreviewedSIes
dc.description.projectMinisterio de Economía, Industria y Competitividad (Grant AYA2017-87515-P)es
dc.description.projectJunta de Castilla y León (Ref. project VA010G18)es
dc.identifier.essn1365-2966es
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional*
dc.type.hasVersioninfo:eu-repo/semantics/acceptedVersiones


Ficheros en el ítem

Thumbnail

Este ítem aparece en la(s) siguiente(s) colección(ones)

Mostrar el registro sencillo del ítem