R-matrix calculations along iso-electronic sequences

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R-matrix calculations along iso-electronic sequences Michael Witthoeft, Allan Whiteford, Nigel Badnell University of Strathclyde Introduction Robust suite of R-matrix codes (LS, ICFT, BreitPauli, Dirac) + Increased availability of parallel computers Ability to efficiently calculate collision strengths along an iso-electronic sequence Need: • an easier way to run an R-matrix calculation • to be able to quickly analyze the large amount of data R-matrix Script • A flexible Perl script to automate an R-matrix calculation • works for serial or parallel machines • calculation sequence: • AUTOSCTRUCTURE (structure and high-energy limit points) • ICFT R-matrix calculation • produce adf04 file (fully commented) • supports radiation damping • no Auger damping yet R-matrix Analysis Package (RAP) RAP base package: • a set of Python routines that read and manipulate the R-matrix results • reads in: • adf04 files • AUTOSTRUCTURE output files (GF values) • TCCDW.DAT files (term coupling coefficients) RAP GUI: • Graphical interface to the routines in the base package • Produce data files and plots of energies and effective collision strengths F-like Sequence • ICFT calculation with 87 terms and 195 levels. • contains the configurations – 2s2 2p5 (two fine-structure levels) – 2s 2p6 – 2s2 2p4 3l – 2s 2p5 3l – 2s2 2p4 4l • Scaling parameters for the structure are optimized for each individual ion. • All ions from Ne+ to Kr27+ 5 x 10-6 1 x 10-5 5 x 10-5 1 x 10-4 Z 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 Structure Energy Levels Shown here are the energy levels for several ions along the sequence. We see that the levels scale as z2 for the higher-Z ions. Energy Levels Here are the energy levels for three ions split by configuration. Notice that the mixing between configurations decreases with increasing charge. Energy of the fine-structure level compared to NIST 2s2 2p5 2P1/2 2s2 2p4 3s 4P5/2 compared to NIST This is representative of the other energy levels GF value: 2s2 2p5 2P3/2 – 2s 2p6 2S1/2 GF value: 2s2 2p5 2P3/2 – 2s2 2p4 3s 2P3/2 GF value: 2s2 2p5 2P3/2 – 2s2 2p4 3d 2D5/2 Resonance Resolution Si5+ Two energy meshes were used: 10-4 and 5x10-5. A ratio plot gives a good overview of the convergence of the effective collision strengths with respect to energy mesh for a given temperature. Only 1.2% of the transitions disagree by more than 10% between the two calculations. Si5+ transitions from the ground term The agreement for all of the these transitions is better than 10%. Si5+ Here is another ratio plot, but now we are plotting as a function of transition energy. The transitions on the right are the low-tohigh transitions. The ones on the left are the high-to-high transitions. Ti13+ 2s2 2p5 2P3/2 - 2s2 2p4 3s 2S1/2 Comparisons Fine-structure transition: Present calculations compared against Berrington et al. (IP XXVIII). Fine-structure transition: T = 104 z12 K Fine-structure transition: T = 103 z12 K 1-2 transition Observe how the resonances move to lower scaled energy as Z increases. The blue lines show 103 and 104 z12 K. Fine-structure: Ne+ Fine-structure: Mg3+ Fine-structure: Si4+ Fine-structure: Fe17+ 2s2 2p5 2P3/2 – 2s 2p6 2S1/2 Ne+ Si5+ Ti13+ Fe17+ 2s2 2p5 2P3/2 – 2s2 2p4 3s 4P5/2 Ne+ Ti13+ Fe17+ Ni21+ Conclusions • Complete F-like sequence has been calculated • Ne, Na, and Mg will be recalculated using observed energies • Sequences in progress: H-, He-, and Li-like (using radiation damping) • Next sequences will be the Ne- and Na-like

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