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 …

Abstract Changes in the Earth's rotation are deeply connected to fluid dynamical processes
in the outer core. This connection can be explored by studying the associated Earth …

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 …

This paper examines the energetics of a convective flow subject to an oscillation with a
period much smaller than the convective time-scale, allowing for compressibility and uniform …

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 …

All the studies of the interaction between tides and a convective flow assume that the large-
scale tides can be described as a mean shear flow that is damped by small-scale fluctuating …

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 …

The interaction between equilibrium tides and convection in stellar envelopes is often
considered important for tidal evolution in close binary and extrasolar planetary systems. Its …