Laboratory Benchmark of $n\geq4$ Dielectronic Recombination Satellites of Fe XVII
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| Format: | Preprint |
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2024
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| author | Grell, Gabriel J. Leutenegger, Maurice A. Amaro, Pedro López-Urrutia, José R. Crespo Shah, Chintan |
| author_facet | Grell, Gabriel J. Leutenegger, Maurice A. Amaro, Pedro López-Urrutia, José R. Crespo Shah, Chintan |
| contents | We calculated cross sections for the dielectronic recombination (DR) satellite lines of Fe XVII and benchmarked our predictions with experimental cross sections of Fe XVII resonances that were mono-energetically excited in an electron beam ion trap. We extend the benchmark to all resolved DR and direct electron-impact excitation (DE) channels in the experimental dataset, specifically the $n\geq4$ DR resonances of Fe XVII, complementing earlier investigations of $n=3$ channels. Our predictions overestimate by 20-25$\%$ the DR and DE absolute cross sections for the higher $n$ complexes when using the same methods as in previous works. However, we achieve agreement within $\sim$10$\%$ of the experimental results by an approach in which we "forward fold" the predicted cross sections with the spread of the electron-beam energy and the photon-energy resolution of our experiment. We then calculated rate coefficients from the experimental and theoretical cross sections, finding departures of $10-20\%$ from the rates found in the OPEN-ADAS atomic database. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2402_08767 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Laboratory Benchmark of $n\geq4$ Dielectronic Recombination Satellites of Fe XVII Grell, Gabriel J. Leutenegger, Maurice A. Amaro, Pedro López-Urrutia, José R. Crespo Shah, Chintan Atomic Physics High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics Plasma Physics We calculated cross sections for the dielectronic recombination (DR) satellite lines of Fe XVII and benchmarked our predictions with experimental cross sections of Fe XVII resonances that were mono-energetically excited in an electron beam ion trap. We extend the benchmark to all resolved DR and direct electron-impact excitation (DE) channels in the experimental dataset, specifically the $n\geq4$ DR resonances of Fe XVII, complementing earlier investigations of $n=3$ channels. Our predictions overestimate by 20-25$\%$ the DR and DE absolute cross sections for the higher $n$ complexes when using the same methods as in previous works. However, we achieve agreement within $\sim$10$\%$ of the experimental results by an approach in which we "forward fold" the predicted cross sections with the spread of the electron-beam energy and the photon-energy resolution of our experiment. We then calculated rate coefficients from the experimental and theoretical cross sections, finding departures of $10-20\%$ from the rates found in the OPEN-ADAS atomic database. |
| title | Laboratory Benchmark of $n\geq4$ Dielectronic Recombination Satellites of Fe XVII |
| topic | Atomic Physics High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics Plasma Physics |
| url | https://arxiv.org/abs/2402.08767 |