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 …

A large fraction of known exoplanets have short orbital periods where tidal excitation of
gravity waves within the host star causes the planets' orbits to decay. We study the effects of …

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 …

Binary stars evolve into chemically peculiar objects and are a major driver of the galactic
enrichment of heavy elements. During their evolution they undergo interactions, including …

Tidal forces are important for understanding how close binary stars and compact
exoplanetary systems form and evolve. However, tides are difficult to model, and significant …

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 …