Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3858
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dc.contributor.authorRay, H-
dc.date.accessioned2008-09-23T15:23:54Z-
dc.date.available2008-09-23T15:23:54Z-
dc.date.issued2003-02-
dc.identifier.citationAstrophysics and Space Science, Vol. 283, No. 3, pp. 415 - 436en
dc.identifier.issn0004 - 640X-
dc.identifier.urihttp://hdl.handle.net/2248/3858-
dc.descriptionRestricted Access-
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractAccurate theoretical data for the transition probabilities are highly demanding in astrophysics and in the study of plasma in astrophysical objects and fusion devices. Na-like highly stripped ions of iron group, specially NiXVIII is very important in this respect. A highly improved basis in a relativistic many-body coupled-cluster method (CCM) to include correlation properly is employed to calculate excitation energies, the electric quadrupole (E2) transition line strengths and transition probabilities for NiXVIII. The effect of correlation is studied thoroughly. The present improved data for different atomic/ionic properties are compared with the available theoretical and/or experimental data and they are in agreement. Some E2 transition data are reported for the first time.en
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://dx.doi.org/10.1023/A:1021628816642en
dc.rights© Springer-
dc.subjectE2-transitionen
dc.subjectStellar Chemical Compositionen
dc.subjectAstrophysical Plasmaen
dc.subjectFusion Deviceen
dc.titleE2-transition probabilities for NiXVIIIen
dc.typeArticleen
Appears in Collections:IIAP Publications

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