Considering the full spectrum of linear unstable modes allows the turbulent diffusion coefficient in thermohaline convection to self-consistently interpolate between previously discrepant theoretical scalings.
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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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Unifying Transport Models of Thermohaline Convection in Stars
Considering the full spectrum of linear unstable modes allows the turbulent diffusion coefficient in thermohaline convection to self-consistently interpolate between previously discrepant theoretical scalings.
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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.