Abstract
In the present work, we report an investigation on the importance of using realistic partition functions in the opacity calculations of lanthanide ions whether they are moderately or lowly ionized. In order to do this, atomic data for various moderately charged samarium (Sm V–XI) and lowly charged neodymium (Nd II–IV) ions were calculated by the pseudo-relativistic Hartree–Fock method (HFR) and then, used to compute the expansion opacities for conditions characterizing the ejecta of kilonovae observed as a result of neutron star mergers, with a particular attention given to the partition function computations.
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Data Availability Statement
This manuscript has no associated data or the data will not be deposited. [Authors’ comment: The aim of the present work being to investigate and discuss the impact of the use of realistic partition functions on opacities, the very numerous atomic parameters obtained in our calculations are not tabulated in this paper. These are available on request from the authors.]
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Acknowledgements
HCG is a holder of a FRIA fellowship, while PP and PQ are, respectively, Research Associate and Research Director of the Belgian Fund for Scientific Research F.R.S.-FNRS. JD has received funding from the FWO and F.R.S.-FNRS under the Excellence of Science (EOS) programme (Nos. O.0004.22 and O022818F). Computational resources have been provided by the Consortium des Equipements de Calcul Intensif (CECI), funded by the F.R.S. -FNRS under Grant No. 2.5020.11 and by the Walloon Region of Belgium.
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Carvajal Gallego, H., Deprince, J., Godefroid, M. et al. On the importance of using realistic partition functions in kilonova opacity calculations. Eur. Phys. J. D 77, 72 (2023). https://doi.org/10.1140/epjd/s10053-023-00638-0
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DOI: https://doi.org/10.1140/epjd/s10053-023-00638-0