A new 3D non-LTE Ag I model atom yields a solar silver abundance of 1.15 ± 0.08, raising the prior value by 0.19 dex and shrinking the meteoritic offset to 0.06 dex.
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The paper identifies five major open questions in nucleosynthesis and notes new tools such as large-scale chemical cartography, astrometric and asteroseismic data, gravitational wave detections, 3-D simulations, and improved lab measurements that will aid progress.
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Ag I model atom and the 3D non-LTE solar silver abundance
A new 3D non-LTE Ag I model atom yields a solar silver abundance of 1.15 ± 0.08, raising the prior value by 0.19 dex and shrinking the meteoritic offset to 0.06 dex.
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The Origin of Elements Across Cosmic Time: Astro2020 Science White Paper
The paper identifies five major open questions in nucleosynthesis and notes new tools such as large-scale chemical cartography, astrometric and asteroseismic data, gravitational wave detections, 3-D simulations, and improved lab measurements that will aid progress.