Comprehensive Laboratory Benchmark of K-shell Dielectronic Satellites of Fe XXV-XXI Ions

Fuente: arXiv
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Autores principales: Shah, Chintan, Amaro, Pedro, Grilo, Filipe, Gu, Ming Feng, Gu, Liyi, Santos, José Paulo, Porter, F. Scott, Pfeifer, Thomas, Leutenegger, Maurice A., López-Urrutia, José R. Crespo
Formato: Preprint
Publicado: 2025
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author Shah, Chintan
Amaro, Pedro
Grilo, Filipe
Gu, Ming Feng
Gu, Liyi
Santos, José Paulo
Porter, F. Scott
Pfeifer, Thomas
Leutenegger, Maurice A.
López-Urrutia, José R. Crespo
author_facet Shah, Chintan
Amaro, Pedro
Grilo, Filipe
Gu, Ming Feng
Gu, Liyi
Santos, José Paulo
Porter, F. Scott
Pfeifer, Thomas
Leutenegger, Maurice A.
López-Urrutia, José R. Crespo
contents We report on comprehensive laboratory studies of the K-shell dielectronic recombination (DR) resonances of Fe XXV - XXI ions that prominently contribute to the hard X-ray spectrum of hot astrophysical plasmas. By scanning a monoenergetic electron beam to resonantly excite trapped Fe ions in an electron beam ion trap, and achieving a high electron-ion collision energy resolution of ~7 eV, we resolve their respective KL$n$ satellites up to n'=11. By normalization to known radiative recombination cross sections we also determine their excitation cross sections and that of the continuum with uncertainties below 15%, and verify our results with an independent normalization based on previous measurements. Our experimental data excellently confirm the accuracy and suitability of distorted-wave calculations obtained with the Flexible Atomic Code (FAC) for modeling astrophysical and fusion plasmas.
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id arxiv_https___arxiv_org_abs_2505_14833
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Comprehensive Laboratory Benchmark of K-shell Dielectronic Satellites of Fe XXV-XXI Ions
Shah, Chintan
Amaro, Pedro
Grilo, Filipe
Gu, Ming Feng
Gu, Liyi
Santos, José Paulo
Porter, F. Scott
Pfeifer, Thomas
Leutenegger, Maurice A.
López-Urrutia, José R. Crespo
Atomic Physics
High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
Solar and Stellar Astrophysics
Plasma Physics
We report on comprehensive laboratory studies of the K-shell dielectronic recombination (DR) resonances of Fe XXV - XXI ions that prominently contribute to the hard X-ray spectrum of hot astrophysical plasmas. By scanning a monoenergetic electron beam to resonantly excite trapped Fe ions in an electron beam ion trap, and achieving a high electron-ion collision energy resolution of ~7 eV, we resolve their respective KL$n$ satellites up to n'=11. By normalization to known radiative recombination cross sections we also determine their excitation cross sections and that of the continuum with uncertainties below 15%, and verify our results with an independent normalization based on previous measurements. Our experimental data excellently confirm the accuracy and suitability of distorted-wave calculations obtained with the Flexible Atomic Code (FAC) for modeling astrophysical and fusion plasmas.
title Comprehensive Laboratory Benchmark of K-shell Dielectronic Satellites of Fe XXV-XXI Ions
topic Atomic Physics
High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
Solar and Stellar Astrophysics
Plasma Physics
url https://arxiv.org/abs/2505.14833