Oxygen Opacity Measurements at High-Energy-Density Conditions

We present the first benchmark measurements of oxygen opacity at high-energy-density, crucial for understanding stellar interiors. A 3-5-μm thick SiO_{2} sample was heated using a Z facility x-ray source, and opacity was measured in the 5-19.5 Å range with multiple spectrometers. The electron temperature and density inferred from Si K-shell spectra were 148±4 eV and 8.6±1.4× 10^{21} cm^{-3}, respectively. Six experiments showed opacity reproducibility within ±15% and 5%-25% opacity uncertainty. Measured oxygen opacity and seven different opacity models exhibit extraordinary overall agreement. Discrepancies near the H-like photon ionization threshold and in certain spectral lines suggest the need for model refinements.

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Publication Details

Journal
Physical Review Letters
Published
2025-11-12
DOI
https://doi.org/10.1103/n2k6-358d
Citations
2
Primary Topic
Astronomy and Astrophysical Research
Type
article
Field-Weighted Citation Impact
2.38

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article

Oxygen Opacity Measurements at High-Energy-Density Conditions

C. Blancard, Daniel Åberg, Ming Feng Gu, Carlos Monton et al.
2 citations
Physical Review Letters
Astronomy and Astrophysical Research
2.38
article

Oxygen Opacity Measurements at High-Energy-Density Conditions

C. Blancard, Daniel Åberg, Ming Feng Gu, Carlos Monton, Guillaume Loisel, Daniel Mayes, R. Santana, F. Gilleron, G. S. Dunham, H. Huang, Taisuke Nagayama, Thomas Gomez, Ph. Cossé, J. Colgan, Carlos A. Iglesias, Jean‐Christophe Pain, G. Faussurier, Christopher J. Fontes, Stephanie B. Hansen, I. Golovkin, Bruce W Wilson, J. E. Bailey
article en
2 citations

Abstract

We present the first benchmark measurements of oxygen opacity at high-energy-density, crucial for understanding stellar interiors. A 3-5-μm thick SiO_{2} sample was heated using a Z facility x-ray source, and opacity was measured in the 5-19.5 Å range with multiple spectrometers. The electron temperature and density inferred from Si K-shell spectra were 148±4 eV and 8.6±1.4× 10^{21} cm^{-3}, respectively. Six experiments showed opacity reproducibility within ±15% and 5%-25% opacity uncertainty. Measured oxygen opacity and seven different opacity models exhibit extraordinary overall agreement. Discrepancies near the H-like photon ionization threshold and in certain spectral lines suggest the need for model refinements.

Physical Review LettersVol. 135(20)
Lawrence Livermore National Laboratory (US), Los Alamos National Laboratory (US), University of Colorado Boulder (US), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Université Paris-Saclay (FR), University of Colorado System (US), CEA DAM Île-de-France (FR), Sandia National Laboratories (US), Prism Computational Sciences (United States) (US), General Atomics (United States) (US), The University of Texas at Austin (US)
U.S. Department of Energy, Ohio State University, National Nuclear Security Administration, Observatoire de Paris, Université de Recherche Paris Sciences et Lettres, Lawrence Livermore National Laboratory, Sandia National Laboratories, Los Alamos National Laboratory
Openalex Percentile: Top 9%
Astronomy and Astrophysical Research
2.38
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