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Effects of configuration interaction on photoabsorption spectra in the continuum

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dc.contributor.author Komninos, Y en
dc.contributor.author Nicolaides, CA en
dc.date.accessioned 2014-03-01T01:20:17Z
dc.date.available 2014-03-01T01:20:17Z
dc.date.issued 2004 en
dc.identifier.issn 1050-2947 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/15886
dc.subject.classification Optics en
dc.subject.classification Physics, Atomic, Molecular & Chemical en
dc.subject.other Absorption en
dc.subject.other Electric excitation en
dc.subject.other Electron energy levels en
dc.subject.other Electronic structure en
dc.subject.other Ionizing radiation en
dc.subject.other Laser beam effects en
dc.subject.other Phase shift en
dc.subject.other Photons en
dc.subject.other Resonance en
dc.subject.other Autoionization en
dc.subject.other Configuration interaction in the continuum (CIC) theory en
dc.subject.other Dipole transitions en
dc.subject.other Photoabsorption en
dc.subject.other Photoionization en
dc.title Effects of configuration interaction on photoabsorption spectra in the continuum en
heal.type journalArticle en
heal.identifier.primary 10.1103/PhysRevA.70.042507 en
heal.identifier.secondary http://dx.doi.org/10.1103/PhysRevA.70.042507 en
heal.identifier.secondary 042507 en
heal.language English en
heal.publicationDate 2004 en
heal.abstract It is pointed out that the proper interpretation of a recently published experimental spectrum from the multilaser photoionization of Sr [Eichmann et al., Phys. Rev. Lett. 90, 233004 (2003)] must account for a radiative transition between two autoionizing states. The application of orthonormality selection rules and of configuration-interaction theory involving the continuous spectrum and the quasicontinuum of the upper part of Rydberg series explains quantitatively the appearance, the shape, and the variation of heights of the observed peaks of resonances. en
heal.publisher AMER PHYSICAL SOC en
heal.journalName Physical Review A - Atomic, Molecular, and Optical Physics en
dc.identifier.doi 10.1103/PhysRevA.70.042507 en
dc.identifier.isi ISI:000225322500043 en
dc.identifier.volume 70 en
dc.identifier.issue 4 en
dc.identifier.spage 042507 en
dc.identifier.epage 1-042507-4 en


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