论文标题
Palatini重力的巨型行星形成
Giant planet formation in Palatini gravity
论文作者
论文摘要
在Palatini重力的背景下，研究了Jovian行星形成的增生模型的某些部分。我们主要关注临界核心质量，也就是说，对于该行星的包膜没有静水平衡溶液，这是失控积聚的起点。我们还讨论了一个行星所需的条件，以便它可以在固体芯周围具有巨大的气态信封。
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.
