Generalized flux-weighted boundary injection rules in collisionless kinetic models yield non-thermal stationary states with non-monotonic profiles, recovering thermal equilibrium only for the standard case.
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The Bern Model has incorporated MHD disk evolution, pebble accretion, and improved interiors, yielding quantitative matches to exoplanet mass functions, radius distributions, and system architectures.
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Generalized flux-weighted boundary walls in kinetic models
Generalized flux-weighted boundary injection rules in collisionless kinetic models yield non-thermal stationary states with non-monotonic profiles, recovering thermal equilibrium only for the standard case.
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The formation of planetary systems: physics, populations, and architectures
The Bern Model has incorporated MHD disk evolution, pebble accretion, and improved interiors, yielding quantitative matches to exoplanet mass functions, radius distributions, and system architectures.