arXiv · astro-ph/0309175
Is planetary migration inevitable?
Abstract
According to current theories, tidal interactions between a disk and an embedded planet may lead to the rapid migration of the protoplanet on a timescale shorter than the disk lifetime or estimated planetary formation timescales. Therefore, planets can form only if there is a mechanism to hold at least some of the cores back on their way in. Once a giant planet has assembled, there also has to be a mechanism to prevent it from migrating down to the disk center. This paper reviews the different mechanisms that have been proposed to stop or slow down migration.
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Caroline E. J. M. L. J. Terquem. 2003-09-05. Is planetary migration inevitable?. https://arxiv.org/abs/astro-ph/0309175
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