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astro-ph.EP2023
Orbital Decay of Hot Jupiters due to Weakly Nonlinear Tidal Dissipation
Nevin N. Weinberg, Niyousha Davachi, Reed Essick +3
We study tidal dissipation in hot Jupiter host stars due to the nonlinear damping of tidally driven -modes, extending the calculations of Essick & Weinberg (2016) to a wide vari…
astro-ph.EP2017★ 65 cited
Tidal Dissipation in WASP-12
Nevin N. Weinberg, Meng Sun, Phil Arras +1
WASP-12 is a hot Jupiter system with an orbital period of , making it one of the shortest-period giant planets known. Recent transit timing observations by Mac…
astro-ph.EP2015★ 119 cited
Orbital decay of hot Jupiters due to nonlinear tidal dissipation within solar-type hosts
Reed Essick, Nevin N. Weinberg
We study the orbital evolution of hot Jupiters due to the excitation and damping of tidally driven -modes within solar-type host stars. Linearly resonant -modes (the dynamica…