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Photoionization of Aluminum-Like P2+ and Magnesium-Like P3+ by the Screening Constant by Unit Nuclear Charge Method

Received: 5 November 2019    Accepted: 25 November 2019    Published: 4 December 2019
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Abstract

In the present work, accurate high lying single photoionization resonance energies for Aluminium-like P2+ and magnesium-like P3+ are reported. Calculations are performed in the framework of the Screening Constant by Unit Nuclear Charge (SCUNC) formalism. The resonance energies and quantum defects obtained compared very well with experimental data of Hernández et al., (2015) along with DARC, Dirac Atomic R-matrix Codes computations of Wang et al., (2016). Analysis of the present results is achieved in the framework of the standard quantum-defect theory and of the SCUNC-procedure based on the calculation of the effective charge. It is demonstrated that the SCUNC-method can be used to assist fruitfully experiments for identifying narrow resonance energies due to overlapping peaks. New precise data for Aluminium-like P2+ and magnesium-like P3+ ions are presented as useful guidelines for investigators focusing their challenge on the Photoionization of aluminum-like P2+ and magnesium-like P3+ heavy charged ions in connection with their application in laboratory, astrophysics, and plasma physics. In addition, our predicted data up to n = 30 may be of great importance for the atomic physics community in connection with the determination of accurate abundances for phosphorus in the solar photosphere, in solar twins, in the infrared spectrum of Messier 77 galaxy (NGC1068).

Published in Nuclear Science (Volume 4, Issue 4)
DOI 10.11648/j.ns.20190404.11
Page(s) 34-43
Creative Commons

This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.

Copyright

Copyright © The Author(s), 2024. Published by Science Publishing Group

Keywords

Photoionization, Resonance Energies, Rydberg Series, Ground State, Metastable State, SCUNC

References
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[8] Hubrig S., et al., 2009. Astron. Astrophys. 499, 865.
[9] Hernández L., et al., 2015. J. Quant. Spectrosc. Radiat. Transf. 159, 80.
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[11] Wang, H. B., et al., 2016. Eur. Phys. J. D. 70, 122.
[12] C. Mendoza, Atomic Datafromthe Opacity Project, http://cdsweb.u-strasbg.fr/topbase/xsections.html.
[13] Sakho I., 2018. The Screening constant by unit nuclear charge method, Description & application to the photoionization of atomic systems ISTE Science Publishing Ltd, London and John Wiley & Sons, Inc., USA.
[14] I. Sakho., 2017. At. Data. Nuc. Data Tables 117-118.
[15] I. Sakho., 2018. J. Electron Spectro & Related Phenomena 222, 40.
[16] I. Sakho., 2014. At. Data. Nuc. Data Tables 100 - 297
[17] Ba, M. D., et al., 2018. Radiat. Phys. Chem. 153, 111.
[18] Badiane J. K., et al., 2019. Rad. Phys. Chem. 158, 17.
[19] Khatri, I., et al., 2016. Radiat. Phys. Chem. 130, 208.
[20] Kramida A, Ralchenko Yu, Reader J., NIST ASD Team (2013). NIST Atomic Spectra Data base (ver. 5.1), [Online]. Available: http://physics.nist.gov/asd [2014 February 25]. National Institute of Standards and Technology, Gaithersburg, MD.
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    Momar Talla Gning, Jean Kouhissoré Badiane, Abdourahmane Diallo, Mamadou Diouldé Ba, Ibrahima Sakho. (2019). Photoionization of Aluminum-Like P2+ and Magnesium-Like P3+ by the Screening Constant by Unit Nuclear Charge Method. Nuclear Science, 4(4), 34-43. https://doi.org/10.11648/j.ns.20190404.11

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    ACS Style

    Momar Talla Gning; Jean Kouhissoré Badiane; Abdourahmane Diallo; Mamadou Diouldé Ba; Ibrahima Sakho. Photoionization of Aluminum-Like P2+ and Magnesium-Like P3+ by the Screening Constant by Unit Nuclear Charge Method. Nucl. Sci. 2019, 4(4), 34-43. doi: 10.11648/j.ns.20190404.11

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    AMA Style

    Momar Talla Gning, Jean Kouhissoré Badiane, Abdourahmane Diallo, Mamadou Diouldé Ba, Ibrahima Sakho. Photoionization of Aluminum-Like P2+ and Magnesium-Like P3+ by the Screening Constant by Unit Nuclear Charge Method. Nucl Sci. 2019;4(4):34-43. doi: 10.11648/j.ns.20190404.11

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  • @article{10.11648/j.ns.20190404.11,
      author = {Momar Talla Gning and Jean Kouhissoré Badiane and Abdourahmane Diallo and Mamadou Diouldé Ba and Ibrahima Sakho},
      title = {Photoionization of Aluminum-Like P2+ and Magnesium-Like P3+ by the Screening Constant by Unit Nuclear Charge Method},
      journal = {Nuclear Science},
      volume = {4},
      number = {4},
      pages = {34-43},
      doi = {10.11648/j.ns.20190404.11},
      url = {https://doi.org/10.11648/j.ns.20190404.11},
      eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ns.20190404.11},
      abstract = {In the present work, accurate high lying single photoionization resonance energies for Aluminium-like P2+ and magnesium-like P3+ are reported. Calculations are performed in the framework of the Screening Constant by Unit Nuclear Charge (SCUNC) formalism. The resonance energies and quantum defects obtained compared very well with experimental data of Hernández et al., (2015) along with DARC, Dirac Atomic R-matrix Codes computations of Wang et al., (2016). Analysis of the present results is achieved in the framework of the standard quantum-defect theory and of the SCUNC-procedure based on the calculation of the effective charge. It is demonstrated that the SCUNC-method can be used to assist fruitfully experiments for identifying narrow resonance energies due to overlapping peaks. New precise data for Aluminium-like P2+ and magnesium-like P3+ ions are presented as useful guidelines for investigators focusing their challenge on the Photoionization of aluminum-like P2+ and magnesium-like P3+ heavy charged ions in connection with their application in laboratory, astrophysics, and plasma physics. In addition, our predicted data up to n = 30 may be of great importance for the atomic physics community in connection with the determination of accurate abundances for phosphorus in the solar photosphere, in solar twins, in the infrared spectrum of Messier 77 galaxy (NGC1068).},
     year = {2019}
    }
    

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  • TY  - JOUR
    T1  - Photoionization of Aluminum-Like P2+ and Magnesium-Like P3+ by the Screening Constant by Unit Nuclear Charge Method
    AU  - Momar Talla Gning
    AU  - Jean Kouhissoré Badiane
    AU  - Abdourahmane Diallo
    AU  - Mamadou Diouldé Ba
    AU  - Ibrahima Sakho
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    PY  - 2019
    N1  - https://doi.org/10.11648/j.ns.20190404.11
    DO  - 10.11648/j.ns.20190404.11
    T2  - Nuclear Science
    JF  - Nuclear Science
    JO  - Nuclear Science
    SP  - 34
    EP  - 43
    PB  - Science Publishing Group
    SN  - 2640-4346
    UR  - https://doi.org/10.11648/j.ns.20190404.11
    AB  - In the present work, accurate high lying single photoionization resonance energies for Aluminium-like P2+ and magnesium-like P3+ are reported. Calculations are performed in the framework of the Screening Constant by Unit Nuclear Charge (SCUNC) formalism. The resonance energies and quantum defects obtained compared very well with experimental data of Hernández et al., (2015) along with DARC, Dirac Atomic R-matrix Codes computations of Wang et al., (2016). Analysis of the present results is achieved in the framework of the standard quantum-defect theory and of the SCUNC-procedure based on the calculation of the effective charge. It is demonstrated that the SCUNC-method can be used to assist fruitfully experiments for identifying narrow resonance energies due to overlapping peaks. New precise data for Aluminium-like P2+ and magnesium-like P3+ ions are presented as useful guidelines for investigators focusing their challenge on the Photoionization of aluminum-like P2+ and magnesium-like P3+ heavy charged ions in connection with their application in laboratory, astrophysics, and plasma physics. In addition, our predicted data up to n = 30 may be of great importance for the atomic physics community in connection with the determination of accurate abundances for phosphorus in the solar photosphere, in solar twins, in the infrared spectrum of Messier 77 galaxy (NGC1068).
    VL  - 4
    IS  - 4
    ER  - 

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Author Information
  • Department of Experiential Sciences, UFR Sciences and Technologies, University of Thies, Thies, Senegal

  • Department of Physics, UFR Sciences and Technologies, University Assane Seck of Ziguinchor, Ziguinchor, Senegal

  • Department of Physics, UFR Sciences and Technologies, University Assane Seck of Ziguinchor, Ziguinchor, Senegal

  • Department of Physics, UFR Sciences and Technologies, University Assane Seck of Ziguinchor, Ziguinchor, Senegal

  • Department of Experiential Sciences, UFR Sciences and Technologies, University of Thies, Thies, Senegal

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