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Relativistic R-matrix calculations for L-shell photoionization cross sections of C Ⅱ |
Lu-You Xie(颉录有)1, Qian-Qian Man(满倩倩)1, Jian-Guo Wang(王建国)2, Yi-Zhi Qu(屈一至)3, Chen-Zhong Dong(董晨钟)1 |
1 Key Laboratory of Atomic and Molecular Physics & Functional Materials of Gansu Province, College of Physics and Electronic Engineering, Northwest Normal University, Lanzhou 730070, China; 2 Key Laboratory of Computational Physics, Institute of Applied Physics and Computational Mathematics, Beijing 100088, China; 3 College of Material Sciences and Opto-electronic Technology, University of the Chinese Academy of Sciences, Beijing 100049, China |
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Abstract The photoionization cross section of the ground state 2s22p 2P1/2o and the first excited state 2s22p 2P3/2o of C Ⅱ ions are systematically calculated using the fully relativistic R-matrix code DARC. The detailed resonances are presented and identified for the photon energy ranging from threshold (24.38 eV) up to 41.5 eV where the L-shell (2p, 2s) photoionization process is dominant. In the calculations, the relativistic effect and electronic correlation effect are well considered. It is found that the relativistic effect is very important for the light atomic system CⅡ, which accounts for experimentally observed fine structure resonance peaks. A careful comparison is made between the present results and the experimental values, and also other theoretical data available in the literature, showing that good agreement is obtained for the resonance peaks.
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Received: 30 March 2018
Revised: 17 May 2018
Accepted manuscript online:
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PACS:
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32.80.-t
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(Photoionization and excitation)
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31.15.am
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(Relativistic configuration interaction (CI) and many-body perturbation calculations)
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Fund: Project supported by the National Key Research and Development Program of China (Grant No. 2017YFA0402300), the National Natural Science Foundation of China (Grant Nos. U1530142, 11474032, and 11774344), and the Young Teachers Scientific Research Ability Promotion Plan of Northwest Normal University (Grant No. NWNU-LKQN-15-3). |
Corresponding Authors:
Lu-You Xie
E-mail: xiely@nwnu.edu.cn
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Cite this article:
Lu-You Xie(颉录有), Qian-Qian Man(满倩倩), Jian-Guo Wang(王建国), Yi-Zhi Qu(屈一至), Chen-Zhong Dong(董晨钟) Relativistic R-matrix calculations for L-shell photoionization cross sections of C Ⅱ 2018 Chin. Phys. B 27 083201
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[1] |
Gao L C, Zhang D H, Xie L Y, Wang J G, Shi Y L and Dong C Z 2013 J. Phys. B: At. Mol Opt. Phys. 46 175402
|
[2] |
Li C Y, Han X Y, Wang J G and Qu Y Z 2013 Chin. Phys. B 22 0123201
|
[3] |
Davidson K 1972 Astrophys. J. 171 213
|
[4] |
Colgan J, Zhang H L and Fontes C J 2008 Phys. Rev. A 77 062704
|
[5] |
Nazir R T, Bari M A, Bilal M, Sardar S, Nasim M H and Salahuddin M 2017 Chin. Phys. B 26 023102
|
[6] |
Seaton M J 1987 J. Phys. B: At. Mol. Opt. Phys. 20 6363
|
[7] |
The Opacity Project Team 1995 The Opacity Project, Vol. 1 (Bristol, UK: Institute of Physics Publishing)
|
[8] |
Hummer D G, Berrington K A, Eissner W, Pradhan A K, Saraph H E and Tully J A 1993 Astron. Astrophys. 279 298
|
[9] |
Berrington K A and Balance C 2001 J. Phys. B: At. Mol. Opt. Phys. 34 L383
|
[10] |
Kjeldsen H 2006 J. Phys. B: At. Mol. Opt. Phys. 39 R325
|
[11] |
Müller A, Schippers S, Phaneuf R A, Kilcoyne A L D, Bräuning H, Schlachter A S, Lu M and McLaughlin B M 2010 J. Phys. B: At. Mol. Opt. Phys. 43 225201
|
[12] |
Yan Y and Seaton M J 1987 J. Phys. B: At. Mol. Opt. Phys. 20 6409
|
[13] |
Yan Y, Taylor K T and Seaton M J 1987 J. Phys. B: At. Mol. Opt. Phys. 20 6399
|
[14] |
Berrington K A, Burke P G, Dufton P L and Kingston A E 1977 J. Phys. B: At. Mol. Opt. Phys. 10 1465
|
[15] |
Lan V K, Dourneuf M L, Allard N L, Saraph H E and Eissner W 1989 Comput. Phys. Commun. 55 303
|
[16] |
Nahar S N and Pradhan A K 1997 Astrophys. J. Suppl. 111 339
|
[17] |
Nahar S N 1995 Astrophys. J. Suppl. 101 423
|
[18] |
Nahar S N and Pradhan K A 1994 Phys. Rev. A 49 1816
|
[19] |
Nicolosi P and Villoresi P 1998 Phys. Rev. A 58 4985
|
[20] |
Recanatini P, Nicolosi P and Villoresi P 2001 Phys. Rev. A 64 012509
|
[21] |
Kjeldsen H, Folkmann F, Hansen J E, Knudsen H, Rasmussen M S, West J B and Andersen T 1999 Astrophys. J. 524 L143
|
[22] |
Kjeldsen H, Hansen J E, Folkmann F, Knudsen H, West J B and Andersen T 2001 Astrophys. J. Suppl. 135 285
|
[23] |
Berrington K A, Eissner W and Norrington P H 1995 Comput. Phys. Commun. 92 290
|
[24] |
Nahar S N 2002 Phys. Rev. A 65 052702
|
[25] |
Norrington P H 2004 http://www.am.qub.ac.uk/DARC.
|
[26] |
Burke P G and Berrington K A 1993 Atomic and Molecular Processes: An R-Matrix Approach (Bristol, UK: Institute of Physics Publishing)
|
[27] |
Jönsson P, He X, Fischer C F and Grant I P 2007 Comput. Phys. Commun. 177 597
|
[28] |
Grant I P 2007 Relativistic Quantum Theory of Atoms and Molecules (New York: Springer)
|
[29] |
Jönsson P, Parpia F A and C F Fischer 1996 Comput. Phys. Commun. 96 301
|
[30] |
Hasoglu M F, Abdel-Naby Sh A, Gorczyca T W, Drake J J and McLaughlin B M 2010 Astrophys. J. 724 1296
|
[31] |
Wang L G and Zhou X X 2007 Chin. Phys. 16 2361
|
[32] |
Kramida A, Ralchenko Yu, Reader J and NIST ASD Team 2018 NIST Atomic Spectra Database (ver. 5.5.3), [Online] Available: https://physics.nist.gov/asd
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