Published April 2019 | Version Published + Accepted Version
Journal Article Open

Plasma environment effects on K lines of astrophysical interest. I. Atomic structure, radiative rates, and Auger widths of oxygen ions

  • 1. ROR icon University of Mons
  • 2. ROR icon Western Michigan University
  • 3. ROR icon Helmholtz Institute Jena
  • 4. ROR icon Friedrich Schiller University Jena
  • 5. ROR icon California Institute of Technology
  • 6. ROR icon University of Erlangen-Nuremberg
  • 7. ROR icon Goddard Space Flight Center
  • 8. ROR icon University of Liège

Abstract

Aims. In the context of black-hole accretion disks, the main goal of the present study is to estimate the plasma environment effects on the atomic structure and radiative parameters associated with the K-vacancy states in ions of the oxygen isonuclear sequence. Methods. We used a time-averaged Debye–Hückel potential for both the electron–nucleus and the electron–electron interactions implemented in the fully relativistic multiconfiguration Dirac–Fock (MCDF) method. Results. Modified ionization potentials, K thresholds, Auger widths, and radiative transition wavelengths and rates are reported for O I–O VII in plasma environments with electron temperature and density ranges 10^5−10^7 K and 10^(18)−10^(22) cm^(−3).

Additional Information

© 2019 ESO. Article published by EDP Sciences. Received 17 January 2019; Accepted 4 March 2019; Published online 12 April 2019. JD is a Research Fellow of the Belgian Fund for Research in Industry and Agriculture FRIA. PP & PQ are, respectively, Research Associate and Research Director of the Belgian Fund for Scientific Research F.R.S. –FNRS. Financial support from these organizations, as well as from the NASA Astrophysics Research and Analysis Program (grant 80NSSC17K0345) is gratefully acknowledged. We are indebted to Professor Nigel R. Badnell (Strathclyde University, UK) for lengthy and useful discussions on the validity of the Debye –Hückel potential and its implementations in atomic structure calculations. JAG acknowledges support from the Alexander von Humboldt Foundation.

Attached Files

Published - aa35075-19.pdf

Accepted Version - 1903.04429.pdf

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Additional details

Identifiers

Eprint ID
95001
Resolver ID
CaltechAUTHORS:20190425-153726886

Related works

Funding

Fonds pour la Formation à la Recherche dans l'índustrie et dans l'Ágriculture (FRIA-Belgium)
Fonds de la Recherche Scientifique (FNRS)
NASA
80NSSC17K0345
Alexander von Humboldt Foundation

Dates

Created
2019-04-25
Created from EPrint's datestamp field
Updated
2021-11-16
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