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APPLE: An Evolution Code for Modeling Giant Planets
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DOI：10.3847/1538-4357/ad57c3.png)
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Abstract
En 中文
We introduce APPLE, a novel planetary evolution code designed specifically for the study of giant exoplanet and Jovian planet evolution in the era of Galileo, Juno, and Cassini. With APPLE, state-of-the-art equations of state for hydrogen, helium, ice, and rock are integrated with advanced features to treat ice/rock cores and metals in the gaseous envelope; models for helium rain and hydrogen/helium immiscibility; detailed atmosphere boundary tables that also provide self-consistent albedos and spectra; and options to address envelope metal gradients and stably stratified regions. Our hope is that these purpose-built features of APPLE will help catalyze the development of the next generation of giant exoplanet and Jovian planet evolutionary models.
Keywords:
EQUATION-OF-STATE
DOUBLE-DIFFUSIVE CONVECTION
HYDROGEN-HELIUM MIXTURES
LOW-MASS STARS
PHASE-SEPARATION
INTERNAL HEAT
BROWN DWARFS
THERMAL STRUCTURE
LAYER FORMATION
ENERGY-BALANCE
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5.4
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8.3W
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32.0W
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