<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">J P Santos</style></author><author><style face="normal" font="default" size="100%">Madruga, C.</style></author><author><style face="normal" font="default" size="100%">F. Parente</style></author><author><style face="normal" font="default" size="100%">P. Indelicato</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Relativistic transition probabilities for F-like ions with 10⩽Z⩽49</style></title><secondary-title><style face="normal" font="default" size="100%">Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms</style></secondary-title><short-title><style face="normal" font="default" size="100%">The Physics of Highly Charged Ions Proceedings of the Twelfth International Conference on the Physics of Highly Charged Ions (HCI-2004) Twelfth International Conference on the Physics of Highly Charged Ions JPS_Articles</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2005</style></year></dates><urls><web-urls><url><style face="normal" font="default" size="100%">http://www.sciencedirect.com/science/article/pii/S0168583X05003976</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">1–4</style></number><volume><style face="normal" font="default" size="100%">235</style></volume><pages><style face="normal" font="default" size="100%">171-173</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;In the present work we have calculated several relativistic transition probabilities for the F-like ions with 10 less-than-or-equals, slant Z less-than-or-equals, slant 49, in the framework of the Multi-Configuration Dirac–Fock method, for applications on laserphysics and astrophysics. The lines considered correspond to transitions between levels of 2p43s, 2p43p and 2p43d configurations. The spectral fine structure is taken into consideration and the results for individual lines are given.&lt;/p&gt;
</style></abstract><notes><style face="normal" font="default" size="100%">&lt;p&gt;PACS: 31.25.Jf; 32.30.Rj; 32.70.Cs JPS-Ref22&lt;/p&gt;
</style></notes><custom3><style face="normal" font="default" size="100%">papers3://publication/uuid/32327FCC-EB39-4EC6-AC95-B9243E4F0167</style></custom3><label><style face="normal" font="default" size="100%">r02992</style></label></record></records></xml>