Planetary formation tracks on the HR diagram show three branches: ascending during solid accretion with L proportional to T to the 8th for in-situ planetesimals, near-horizontal during gas accretion, and descending during post-accretion cooling.
High Energy Density Physics , year = 2006, publisher =
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SPRAY is the first SPH-based radiation hydrodynamics code for high-intensity laser-plasma interactions, featuring a mesh-free WKB laser energy coupling module and flux-limited diffusion for radiation transport.
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Planetary formation tracks on the Hertzsprung-Russell diagram: Visualising the processes of giant planet growth
Planetary formation tracks on the HR diagram show three branches: ascending during solid accretion with L proportional to T to the 8th for in-situ planetesimals, near-horizontal during gas accretion, and descending during post-accretion cooling.
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SPRAY: A smoothed particle radiation hydrodynamics code for modeling high intensity laser-plasma interactions
SPRAY is the first SPH-based radiation hydrodynamics code for high-intensity laser-plasma interactions, featuring a mesh-free WKB laser energy coupling module and flux-limited diffusion for radiation transport.