Structure and electronic spectra of the (ProQuest: Formulae and/or non-USASCII text omitted)
Ab initio calculations are employed for determining structures, spectroscopic parameters and transitions to the excited electronic states of the astrophysical relevant (ProQuest: Formulae and/or non-USASCII text omitted) anion, which is a potential intermediate of chemical processes involving carbon...
Gespeichert in:
Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2012-08, Vol.424 (2), p.1224 |
---|---|
Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | 2 |
container_start_page | 1224 |
container_title | Monthly notices of the Royal Astronomical Society |
container_volume | 424 |
creator | Hammoutene, D Hochlaf, M Senent, M. L |
description | Ab initio calculations are employed for determining structures, spectroscopic parameters and transitions to the excited electronic states of the astrophysical relevant (ProQuest: Formulae and/or non-USASCII text omitted) anion, which is a potential intermediate of chemical processes involving carbon chains and polycyclic aromatic hydrocarbons. Calculations confirm the prominent stability of linear carbon chain anions which guarantees their formation. The lowest doublet potential energy surface of (ProQuest: Formulae and/or non-USASCII text omitted) displays six isomers, whereas in the lowest quartet potential energy surface, a unique minimum energy geometry is found. The most stable form is the linear anion (ProQuest: Formulae and/or non-USASCII text omitted) [PUBLICATION ABSTRACT] |
doi_str_mv | 10.1111/j.1365-2966.2012.21299.x |
format | Article |
fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_1030258023</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2724721871</sourcerecordid><originalsourceid>FETCH-proquest_journals_10302580233</originalsourceid><addsrcrecordid>eNqNjEFrAjEUhIO00K32PzzoxR42viTd1fUmUtGbsnoryLJG6rLm2eQF_PlVkZ6dywx8MyMEKJTqokEjlcmzVBd5LjUqLbXSRSHPHZH8gyeRIJosHQ2VehGvITSI-Gl0nojvkn2sOXoLlduBbW3NntyhhnC6xgpoD_xjob_0tIo28Bhm5I-xrW6LAXlw5NJNOSmniwWwPTPQ8cBsdx898byv2mDf7t4V77Ov9XSenjz9Xr-2DUXvLmir0KDORqiNeaz1B9JiSk4</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1030258023</pqid></control><display><type>article</type><title>Structure and electronic spectra of the (ProQuest: Formulae and/or non-USASCII text omitted)</title><source>Oxford Journals Open Access Collection</source><source>Wiley Online Library Journals Frontfile Complete</source><creator>Hammoutene, D ; Hochlaf, M ; Senent, M. L</creator><creatorcontrib>Hammoutene, D ; Hochlaf, M ; Senent, M. L</creatorcontrib><description>Ab initio calculations are employed for determining structures, spectroscopic parameters and transitions to the excited electronic states of the astrophysical relevant (ProQuest: Formulae and/or non-USASCII text omitted) anion, which is a potential intermediate of chemical processes involving carbon chains and polycyclic aromatic hydrocarbons. Calculations confirm the prominent stability of linear carbon chain anions which guarantees their formation. The lowest doublet potential energy surface of (ProQuest: Formulae and/or non-USASCII text omitted) displays six isomers, whereas in the lowest quartet potential energy surface, a unique minimum energy geometry is found. The most stable form is the linear anion (ProQuest: Formulae and/or non-USASCII text omitted) [PUBLICATION ABSTRACT]</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1111/j.1365-2966.2012.21299.x</identifier><language>eng</language><publisher>London: Oxford University Press</publisher><subject>Astronomy ; Astrophysics ; Polycyclic aromatic hydrocarbons ; Spectrum analysis</subject><ispartof>Monthly notices of the Royal Astronomical Society, 2012-08, Vol.424 (2), p.1224</ispartof><rights>2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27901,27902</link.rule.ids></links><search><creatorcontrib>Hammoutene, D</creatorcontrib><creatorcontrib>Hochlaf, M</creatorcontrib><creatorcontrib>Senent, M. L</creatorcontrib><title>Structure and electronic spectra of the (ProQuest: Formulae and/or non-USASCII text omitted)</title><title>Monthly notices of the Royal Astronomical Society</title><description>Ab initio calculations are employed for determining structures, spectroscopic parameters and transitions to the excited electronic states of the astrophysical relevant (ProQuest: Formulae and/or non-USASCII text omitted) anion, which is a potential intermediate of chemical processes involving carbon chains and polycyclic aromatic hydrocarbons. Calculations confirm the prominent stability of linear carbon chain anions which guarantees their formation. The lowest doublet potential energy surface of (ProQuest: Formulae and/or non-USASCII text omitted) displays six isomers, whereas in the lowest quartet potential energy surface, a unique minimum energy geometry is found. The most stable form is the linear anion (ProQuest: Formulae and/or non-USASCII text omitted) [PUBLICATION ABSTRACT]</description><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Polycyclic aromatic hydrocarbons</subject><subject>Spectrum analysis</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><recordid>eNqNjEFrAjEUhIO00K32PzzoxR42viTd1fUmUtGbsnoryLJG6rLm2eQF_PlVkZ6dywx8MyMEKJTqokEjlcmzVBd5LjUqLbXSRSHPHZH8gyeRIJosHQ2VehGvITSI-Gl0nojvkn2sOXoLlduBbW3NntyhhnC6xgpoD_xjob_0tIo28Bhm5I-xrW6LAXlw5NJNOSmniwWwPTPQ8cBsdx898byv2mDf7t4V77Ov9XSenjz9Xr-2DUXvLmir0KDORqiNeaz1B9JiSk4</recordid><startdate>20120801</startdate><enddate>20120801</enddate><creator>Hammoutene, D</creator><creator>Hochlaf, M</creator><creator>Senent, M. L</creator><general>Oxford University Press</general><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20120801</creationdate><title>Structure and electronic spectra of the (ProQuest: Formulae and/or non-USASCII text omitted)</title><author>Hammoutene, D ; Hochlaf, M ; Senent, M. L</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_10302580233</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Polycyclic aromatic hydrocarbons</topic><topic>Spectrum analysis</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hammoutene, D</creatorcontrib><creatorcontrib>Hochlaf, M</creatorcontrib><creatorcontrib>Senent, M. L</creatorcontrib><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hammoutene, D</au><au>Hochlaf, M</au><au>Senent, M. L</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Structure and electronic spectra of the (ProQuest: Formulae and/or non-USASCII text omitted)</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><date>2012-08-01</date><risdate>2012</risdate><volume>424</volume><issue>2</issue><spage>1224</spage><pages>1224-</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>Ab initio calculations are employed for determining structures, spectroscopic parameters and transitions to the excited electronic states of the astrophysical relevant (ProQuest: Formulae and/or non-USASCII text omitted) anion, which is a potential intermediate of chemical processes involving carbon chains and polycyclic aromatic hydrocarbons. Calculations confirm the prominent stability of linear carbon chain anions which guarantees their formation. The lowest doublet potential energy surface of (ProQuest: Formulae and/or non-USASCII text omitted) displays six isomers, whereas in the lowest quartet potential energy surface, a unique minimum energy geometry is found. The most stable form is the linear anion (ProQuest: Formulae and/or non-USASCII text omitted) [PUBLICATION ABSTRACT]</abstract><cop>London</cop><pub>Oxford University Press</pub><doi>10.1111/j.1365-2966.2012.21299.x</doi></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0035-8711 |
ispartof | Monthly notices of the Royal Astronomical Society, 2012-08, Vol.424 (2), p.1224 |
issn | 0035-8711 1365-2966 |
language | eng |
recordid | cdi_proquest_journals_1030258023 |
source | Oxford Journals Open Access Collection; Wiley Online Library Journals Frontfile Complete |
subjects | Astronomy Astrophysics Polycyclic aromatic hydrocarbons Spectrum analysis |
title | Structure and electronic spectra of the (ProQuest: Formulae and/or non-USASCII text omitted) |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-03T13%3A55%3A58IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Structure%20and%20electronic%20spectra%20of%20the%20(ProQuest:%20Formulae%20and/or%20non-USASCII%20text%20omitted)&rft.jtitle=Monthly%20notices%20of%20the%20Royal%20Astronomical%20Society&rft.au=Hammoutene,%20D&rft.date=2012-08-01&rft.volume=424&rft.issue=2&rft.spage=1224&rft.pages=1224-&rft.issn=0035-8711&rft.eissn=1365-2966&rft_id=info:doi/10.1111/j.1365-2966.2012.21299.x&rft_dat=%3Cproquest%3E2724721871%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1030258023&rft_id=info:pmid/&rfr_iscdi=true |