We study tidal dissipation in stars with masses in the range 0.1–1.6 M⊙ throughout their
evolution, including turbulent effective viscosity acting on equilibrium tides and inertial …

Tidal interactions between moons and planets can have major effects on the orbits, spins,
and thermal evolution of the moons. In the Saturn system, tidal dissipation in the planet …

Turbulent convection is thought to act as an effective viscosity (ν E) in damping tidal flows in
stars and giant planets. However, the efficiency of this mechanism has long been debated …

Tidal dissipation in star–planet systems can occur through various mechanisms, among
which is the elliptical instability. This acts on elliptically deformed equilibrium tidal flows in …

Tidal dissipation is responsible for circularizing the orbits and synchronizing the spins of
solar-type close binary stars, but the mechanisms responsible are not fully understood …

We simulate the nonlinear hydrodynamical evolution of tidally excited inertial waves in
convective envelopes of rotating stars and giant planets modeled as spherical shells …

Previous studies pointed out that many observed samples of short-period binaries display a
cut-off period, P cut, such that almost all binaries with periods shorter than P cut have …

Although tidal dissipation in binary stars has been studied for over a century, theoretical
predictions have yet to match the observed properties of binary populations. This work …

In close exoplanetary systems, tidal interactions drive orbital and spin evolution of planets
and stars over long time-scales. Tidally forced inertial waves (restored by the Coriolis …

We study how stably stratified or semi-convective layers alter the tidal dissipation rates
associated with the generation of internal waves in planetary interiors. We consider if these …