Thermal tidal torques in rotating hot Jupiters are enhanced by resonances with g-, r-, and inertial modes, producing broad or sharp peaks depending on non-adiabatic effects and differing between prograde and retrograde forcing.
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Thermal Tides in Rotating Hot Jupiters
Thermal tidal torques in rotating hot Jupiters are enhanced by resonances with g-, r-, and inertial modes, producing broad or sharp peaks depending on non-adiabatic effects and differing between prograde and retrograde forcing.