Relativistic energy levels, lifetimes, and transition probabilities for the sodium-like to argon-like sequences
By C. Fischer, G. Tachiev, A. Irimia. 2006
214 citations recorded by the source corpus.
Subfields: Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/63e61b5d19da0ee028c6b1a86cbeb103520ce268
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In Atomic and Molecular Physics, and Optics
In Nuclear and High Energy Physics
Citations in the corpus
- CHIANTI - An atomic database for Emission Lines. Version 8 (2015, methodology): “We have retained the A-values for the allowed and forbidden transitions we had in the previous CHIANTI version, calculated by Froese Fischer et al. (2006) with the ab initio MHCF method, and the Tayal & Gupta (1999) A-values for the decays from the 4d levels.”
- CHIANTI—An Atomic Database for Emission Lines. XV. Version 9, Improvements for the X-Ray Satellite Lines (2019, methodology): “Theoretical energies were taken from the calculations of Froese Fischer et al. (2006).”