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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/66221
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dc.contributor.authorOrnellas, F. R.-
dc.contributor.authorAndreazza, C. M.-
dc.contributor.authorDe Almeida, A. A.-
dc.date.accessioned2014-05-27T11:19:56Z-
dc.date.accessioned2016-10-25T18:16:31Z-
dc.date.available2014-05-27T11:19:56Z-
dc.date.available2016-10-25T18:16:31Z-
dc.date.issued2000-08-01-
dc.identifier.citationAstrophysical Journal Letters, v. 538, n. 2 PART 1, p. 675-683, 2000.-
dc.identifier.issn2041-8205-
dc.identifier.issn2041-8213-
dc.identifier.urihttp://hdl.handle.net/11449/66221-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/66221-
dc.description.abstractThe A2∑+ and Z2∏ electronic states of the SiP species have been investigated theoretically at a very high level of correlation treatment (CASSCF/MRSDCI). Very accurate potential energy curves are presented for both states, as well as the associated spectroscopic constants as derived from the vib-rotational energy levels determined by means of the numerical solution of the radial Schrödinger equation. Electronic transition moment function, oscillator strengths, Einstein coefficients for spontaneous emission, and Franck-Condon factors for the A2∑+-X2∏ system have been calculated. Dipole moment functions and radiative lifetimes for both states have also been determined. Spin-orbit coupling constants are also reported. The radiative lifetimes for the A2∑+ state, taking into account the spin-orbit diagonal correction to the X2∏ state, decrease from a value of 138 ms at v′ = 0 to 0.48 ms at v′ = 8, and, for the X2∏ state, from 2.32 s at v″ = 1 to 0.59 s at v″ = 5. Vibrational and rotational transitions are expected to be relatively strong.en
dc.format.extent675-683-
dc.language.isoeng-
dc.sourceScopus-
dc.subjectISM: molecules-
dc.subjectMolecular data-
dc.subjectMolecular processes-
dc.titleA theoretical study of the A2 ∑+-X2∏ system of the SiP moleculeen
dc.typeoutro-
dc.contributor.institutionUniversidade de São Paulo (USP)-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniversidade de São Paulo Instituto de Química, CP 26077, 05513-970, São Paulo, SP-
dc.description.affiliationUniversidade Estadual Paulista Inst. de Geociencias e Cie. Exatas Depto. Estat., Matemat. Apl. Compl., Rua 10, 2527,13500-230, Rio Claro, SP-
dc.description.affiliationUniversidade de São Paulo Inst. Astron. e Geofísico, Av. Miguel Stéfano, 4200, 04301-904, São Paulo, SP-
dc.description.affiliationUnespUniversidade Estadual Paulista Inst. de Geociencias e Cie. Exatas Depto. Estat., Matemat. Apl. Compl., Rua 10, 2527,13500-230, Rio Claro, SP-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofAstrophysical Journal Letters-
dc.identifier.scopus2-s2.0-0034239636-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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