Abstract
In this paper, transition wavelengths, transition probabilities, absorption oscillator strengths and line strengths for Kα X-rays from P VI to P XIV have been calculated using the multi-configuration Dirac–Fock and relativistic configuration interaction methods. The contributions of the Breit interaction, self-energy and vacuum polarization corrections have been considered in the calculation. The present data are in good agreement with some previous experimental and theoretical values. The data of P VI to P XIV have been ascertained to be reliable by using the ratio of the velocity to length gauge of the transition rate (A L/A V).
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V Lebouteiller, Kuassivi and R Ferlet Astron. Astrophys. 443 509 (2005)
E Caffau, P Bonifacio, R Faraggiana and M steffen Astron. Astrophys. 532 98 (2011)
B C Koo, Y H Lee, D S Moon, S C Yoon and J C Raymond Science 342 6164 (2013)
S R Pottasch, J Bernard-Salas and T L Roellig Astron. Astrophys. 481 393 (2008)
S R Pottasch and J Bernard-Salas Astron. Astrophys. 490 715 (2008)
V A Boiko, A Ya Faenov, S A Pikuz, I Yu Skobelev, A V Vinogradov and E A Yukov J. Phys. B At. Mol. Phys. 10 3387 (1977)
B C Fawcett, R A Hardcastle and G Tondello J. Phys. B At. Mol. Phys. 3 564 (1970)
E V Aglitskii, V A Boiko, S M Zakharov, S A Pikuz and A Y Faenov Sov. J. Quant. Electron. 4 4 (1974)
A J Bearden Rev. Mod. Phys. 39 1 (1967)
W C Martin, R Zalubas and A Musgrove J. Phys. Chem. Ref. Data. 14 751 (1985)
L L House Astrophys. J. Suppl. Ser. 18 155 (1969)
C Laughlin J. Phys. B At. Mol. Phys. 11 L391 (1978)
C D Lin, W R Johnson and A Dalgarno Phys. Rev. A 15 1 (1977)
G W F Drake Phys. Rev. A 19 4 (1979)
G Marcus, E Louzon, Z Henis and S Maman J. Opt. Soc. Am. B 24 1187
E Louzon et al. Laser Part Beams 29 61 (2011)
G A Vergunova et al. Phys. Scr. 55 483 (1997)
A Bartnic et al. Quant. Electron. 25 19 (1995)
H Fiedorwicz, A Bartnik, R Jarocki, M Szczurek and T Wilhein Appl. Phys. B 67 391 (1998)
E Träbert, I A Armour, S Bashkin, N A Jelley, R O’Brien and J D Silver J. Phys. B 12 1665 (1979)
T Mohamed et al. Phys. Rev. A 66 022719 (2002)
B L Deng, G Jiang, L Zhang, X Wang and X-Z Hua Phys. Scr. 85 045303 (2012)
K G Dyall, I P Grant, C T Johnson, F A Parpia and E P Plummer Comput. Phys. Commun. 55 425 (1989)
F A Parpia, C F Fischer and I P Grant Comput. Phys. Commun. 94 249 (1996)
A Stathopoulos and C F Fisher Comput. Phys. Commum. 79 1 (1994)
J Olsen, M R Godefroid, P A Jonsson, P A Malmquist and C F Fisher Phys. Rev. E 52 4499 (1995)
S Song and F Peng J. Phys. B: At. Mol. Opt. Phys. 39 2087 (2006)
L Hao and G Jiang At. Data Nucl. Data Tables 94 739 (2008)
F Hu, G Jiang, W Hong and L Hao Eur. Phys. J. D 49 293 (2008)
H J Hou, G Jiang, F Hu and L Hao At. Data Nucl. Data Tables 95 125 (2009)
L Zhang, G Jiang, L Hao and B L Deng Phys. Scr. 83 025302 (2011)
Acknowledgments
The authors are grateful to Vanderbilt University for providing the GRASPVU program package for free. This work was supported by the National Natural Science Foundation of China under Grant No. 11174213 and by the Education Department of Sichuan Province under Grant No. 14ZB0069 as well as by the Youth Science Foundation of Chengdu University of Technology under Grant No. 2012QJ11.
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Zhu, X.J., Deng, B.L., Zhang, C.Y. et al. Calculations of relativistic configuration interaction for Kα X-ray satellites of phosphorus ions. Indian J Phys 90, 225–231 (2016). https://doi.org/10.1007/s12648-015-0731-7
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DOI: https://doi.org/10.1007/s12648-015-0731-7