| Dr. T.M. Luke
(519) 661-2111, ext. 88796 Room 121 Western Science Centre tluke@julian.uwo.ca Current Research Program: |
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Interpreting these patterns of the observed spectrum depends on a detailed knowledge of radiative transition rates for transitions between excited states of atoms and ions. This can be obtained either by lab measurements or by modelling the atoms mathematically and solving the resulting equations which is what I do. The atoms in the vicinity of iron in the periodic table are of special interest in stellar astrophysics and my present work concentrates on them. The work is very demanding in computing resources and much of its interest, apart from obtaining useful data, lies in developing numerical and computational techniques that will enable us to carry out the calculations efficiently and accurately.
“On the Contribution of an Efficient Basis for CI Calculations: Application to a Spin Forbidden Transition in P II” (with L. LaJohn) J. Phys. B: At. Mol. Opt. Phys. 26 (1993) 863-871.
“Decay Rates and Lifetimes of the 4p6,4 P and 4p6 D Levels of CrII” (with K. Aashamar) J. Phys. B:At. Mol. Opt. Phys. 27 (1994) 1091-1103.
“Relativistic Transition Rates for 3 Quartet Multiplets in Neutral Vanadium” Physica Scripta 54 (1996) 346-351.
“Allowed and forbidden Transitions in Singly Ionized Vanadium” J. Phys. B:At. Mol. Opt. Phys. 30 (1997) 4223-4239.
“Transition Rates in Singly Ionized Titanium”, Can. J. Phys. 77 (1999) 571-583.