IIA Institutional Repository

E2-transition probabilities for NiXVIII

Show simple item record

dc.contributor.author Ray, H
dc.date.accessioned 2008-09-23T15:23:54Z
dc.date.available 2008-09-23T15:23:54Z
dc.date.issued 2003-02
dc.identifier.citation Astrophysics and Space Science, Vol. 283, No. 3, pp. 415 - 436 en
dc.identifier.issn 0004 - 640X
dc.identifier.uri http://hdl.handle.net/2248/3858
dc.description Restricted Access
dc.description The original publication is available at springerlink.com
dc.description.abstract Accurate 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.iso en en
dc.publisher Kluwer Academic Publishers en
dc.relation.uri http://dx.doi.org/10.1023/A:1021628816642 en
dc.rights © Springer
dc.subject E2-transition en
dc.subject Stellar Chemical Composition en
dc.subject Astrophysical Plasma en
dc.subject Fusion Device en
dc.title E2-transition probabilities for NiXVIII en
dc.type Article en


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Browse

My Account