ORBITAL DECAY OF HOT JUPITERS DUE TO NONLINEAR TIDAL DISSIPATION WITHIN SOLAR-TYPE HOSTS
We study the orbital evolution of hot Jupiters due to the excitation and damping of tidally driven g-modes within solar-type host stars. Linearly resonant g-modes (the dynamical tide) are driven to such large amplitudes in the stellar core that they excite a sea of other g-modes through weakly nonli...
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| 格式: | 文件 |
| 语言: | en_US |
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IOP Publishing
2016
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| 在线阅读: | http://hdl.handle.net/1721.1/101660 https://orcid.org/0000-0001-9194-2084 https://orcid.org/0000-0001-8196-9267 |