Download presentation
Presentation is loading. Please wait.
1
R-matrix calculations along iso-electronic sequences
Michael Witthoeft, Allan Whiteford, Nigel Badnell University of Strathclyde
2
Introduction Robust suite of R-matrix codes (LS, ICFT, Breit-Pauli, 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
3
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
4
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
5
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+ 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 36 30 31 32 33 34 35 Z 1 x 10-4 5 x 10-5 1 x 10-5 5 x 10-6
6
Structure
7
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.
8
Energy Levels Here are the energy levels for three ions split by configuration. Notice that the mixing between configurations decreases with increasing charge.
9
Energy of the fine-structure level compared to NIST
2s2 2p5 2P1/2
10
2s2 2p4 3s 4P5/2 compared to NIST This is representative of the other energy levels
11
GF value: 2s2 2p5 2P3/2 – 2s 2p6 2S1/2 relativistic Hartree-Fock calculation
12
GF value: 2s2 2p5 2P3/2 – 2s2 2p4 3s 2P3/2
13
GF value: 2s2 2p5 2P3/2 – 2s2 2p4 3d 2D5/2
14
Resonance Resolution
15
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.
16
Si5+ transitions from the ground term
The agreement for all of the these transitions is better than 10%.
17
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-to-high transitions. The ones on the left are the high-to-high transitions.
18
Ti13+ 2s2 2p5 2P3/2 - 2s2 2p4 3s 2S1/2
19
Comparisons
20
Fine-structure transition:
Present calculations compared against Berrington et al. (IP XXVIII).
21
Fine-structure transition: T = 104 z12 K
22
Fine-structure transition: T = 103 z12 K
23
1-2 transition Observe how the resonances move to lower scaled energy as Z increases. The blue lines show 103 and 104 z12 K.
24
Fine-structure: Ne+
25
Fine-structure: Mg3+
26
Fine-structure: Si4+
27
Fine-structure: Fe17+
28
2s2 2p5 2P3/2 – 2s 2p6 2S1/2 Ne+ Si5+ Ti13+ Fe17+
29
2s2 2p5 2P3/2 – 2s2 2p4 3s 4P5/2 Ne+ Ti13+ Fe17+ Ni21+
30
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
Similar presentations
© 2024 SlidePlayer.com. Inc.
All rights reserved.