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 dam** 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 …