Giant planet formation in Palatini gravity

Aneta Wojnar

doi:10.1103/physrevd.105.124053

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arXiv · 2203.16260

Giant planet formation in Palatini gravity

Aneta Wojnar

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Abstract

Some parts of the accretion model of the jovian planets' formation are studied in the context of Palatini gravity. We mainly focus on the critical core mass, that is, a mass for which there is no hydrostatic equilibrium solution for the planet's envelope, which is a starting point of the runaway accretion. We also discuss the conditions needed to be satisfied by a planet such that it can posses a massive gaseous envelope around a solid core.

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Aneta Wojnar. 2022-03-30. Giant planet formation in Palatini gravity. https://doi.org/10.1103/physrevd.105.124053

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