dielectronic recombination computations of rh pd and ag
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Dielectronic recombination computations of Rh-, Pd- and Ag-like W - PowerPoint PPT Presentation

Introduction Main work Future work Dielectronic recombination computations of Rh-, Pd- and Ag-like W with the FAC code Bowen Li School of Nuclear Science and Technology, Lanzhou University School of Physics, University College Dublin


  1. Introduction Main work Future work Dielectronic recombination computations of Rh-, Pd- and Ag-like W with the FAC code Bowen Li School of Nuclear Science and Technology, Lanzhou University School of Physics, University College Dublin libw@lzu.edu.cn September 14, 2015

  2. Introduction Main work Future work Contents Introduction 1 Main work 2 Rh-like W Pd-like W Ag-like W Future work 3

  3. Introduction Main work Future work DR Process

  4. Introduction Main work Future work DR Process

  5. Introduction Main work Future work Important stages

  6. Introduction Main work Future work 1. DR of Rh-like W

  7. Introduction Main work Future work Published work

  8. Introduction Main work Future work Energy level 9 7 8 1.2 10 1.2 9 6 5 4 10 7 6 8 3 2 4 1.0 5 1.0 3 2 8 4f 2 1=4d 0.8 0.8 8 4f5l 2=4d 1 (E c -E 0 )/E I 8 5s5l 3=4d 0.6 0.6 8 5p5l 4=4d 1 8 4f6l 5=4d 8 5s6l 0.4 6=4d 0.4 8 5d5l 7=4d 8 4f7l W Gd 8=4d 0.2 0.2 8 5p6l 9=4d 8 5f5l 10=4d 0.0 0.0 Figure: Energy levels of doubly excited configurations within the 4d complexes relative to the first ionization limit E I (565 eV for Gd and 1128 eV for W) which is indicated by the dashed line. E 0 is the gound states energy of Pd-like Gd and W.

  9. Introduction Main work Future work Energy level 8 10 1.4 Gd 1.4 W 9 7 10 8 5 9 1.2 1.2 4 5 3 7 4 3 1.0 2 1.0 6 2 (E c -E 0 )/E I 0.8 0.8 6 1 1 1 0.6 0.6 5 4d 10 4f 1=4p 5 4d 9 4f 2 1 6=4p 0.4 5 4d 10 5l 0.4 2=4p 5 4d 9 4f 1 5l 7=4p 5 4d 10 6l 3=4p 5 4d 9 4f 1 6l 8=4p 0.2 5 4d 10 7l 0.2 4=4p 5 4d 9 5s 2 9=4p 5 4d 10 8l 5=4p 5 4d 9 5p 2 10=4p 0.0 0.0 Figure: Energy levels of doubly excited configurations within the 4p complexes relative to the first ionization limit E I (565 eV for Gd and 1128 eV for W) which is indicated by the dashed line. E 0 is the gound states energy of Pd-like Gd and W.

  10. Introduction Main work Future work 4d and 4p complex -9 10 1 1 10 -10 3 ) -1 2 -10 10 s 3 -11 2 Rate coefficients (cm 10 3 4 -11 10 -12 10 -12 10 5 -13 4 10 1 = sum(4p) 1 = sum(4d) 2 = 4p 5 4d 9 4fn l ' ' 8 ' ' 2 = 4d 4fn l 5 10 ' ' -13 3 = 4p 4d n l 10 8 ' ' 3 = 4d 5ln l -14 10 5 9 ' ' 4 = 4p 4d 5ln l 8 ' ' 4 = 4d 6ln l 5 9 ' ' 5 = 4p 4d 6ln l 1 10 100 100010000 1 10 100 100010000 T (eV) T (eV) e e Figure: Partial DR rate coefficients for 4d and 4p core excited complexes of W.

  11. Introduction Main work Future work n dependence Figure: The DR rate coefficients where an incident electron is captured to the different orbitals of W.

  12. Introduction Main work Future work DR rate -9 1 = Total 5 10 1 2 = NRS 3 = RS -1 ) 4 = scale -3 s 5 = sum(4d) -10 10 Rate coefficients (cm 6 = sum(4p) 3 2 5 3 -11 10 6 1 6 4 4 -12 10 2 1 10 100 1000 10000 T e (eV) Figure: Contributions from the RS and NRS transition as well as different core excitations to total DR rate coefficients as a function of Te in Rh-like W.

  13. Introduction Main work Future work Recombination process

  14. Introduction Main work Future work Section conclusions Dielectronic recombination process is important. The 4p complexes contribute is aroud 25% to the total DR rate coefficients. The contributions from NRS transitions are significantly enhanced for W when compared with Gd as a result of lowering of energy levles relative to the ionization limit.

  15. Introduction Main work Future work 2. DR of Pd-like W † Bowen Li et al. in preparing

  16. Introduction Main work Future work Earlier work

  17. Introduction Main work Future work 4d and 4p complex Figure: Contributions from the RS and NRS transition as well as different core excitations to total DR rate coefficients as a function of Te in Pd-like W.

  18. Introduction Main work Future work DR rate Figure: Contributions from the RS and NRS transition as well as different core excitations to total DR rate coefficients as a function of Te in Pd-like W.

  19. Introduction Main work Future work Section conclusions Very big discrepancy with Safronova et al. . Need new experiment or other calculations. ∆ n = 0 and ∆ n = 1 are important.

  20. Introduction Main work Future work 3. DR of Ag-like W † Bowen Li et al. in preparing, without extrapolation

  21. Introduction Main work Future work Energy level 900 800 Relative energy (eV) 700 600 500 400 300 200 s p d f g h s p d f g h Configurations

  22. Introduction Main work Future work Energy level 900 800 Relative energy (eV) 700 600 500 400 300 200 s p d f g h s p d f g h s p d f g h s p d f g h Configurations

  23. Introduction Main work Future work Complex Total -8 10 4f-complex 4d-complex -1 ) 4p-complex -9 -3 s 10 Rate coefficients (cm -10 10 -11 10 -12 10 -13 10 0.1 1 10 100 1000 10000 T e (eV)

  24. Introduction Main work Future work DR rate

  25. Introduction Main work Future work Future work Check the Pd-like W data. Finish the calculations on Ag-like W. ...

  26. Introduction Main work Future work Acknowledgement NWNU: Prof. Chenzhong Dong, as well as other members UCD: Prof. Gerry O’Sullivan I would like to acknowledge support from the Fundamental Research Funds for the Central Universities Grant No. lzujbky-2014-9, International scientific collaboration program by Gansu Provincial Science and Technology Department Grant No. 144WCGA163 and National Natural Science Foundation of China Grant No. 11404152 as well as financial support from a UCD-CSC scholarship award.

  27. Introduction Main work Future work Thank you for your attention!

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