16 citations · 28 across the 3 of their papers we have counts for
5 papers
Layered semi-convection and tides in giant planet interiors - II. Tidal dissipation
Quentin André, Stéphane Mathis, Adrian J. Barker
Recent Juno observations have suggested that the heavy elements in Jupiter could be diluted throughout a large fraction of its gaseous envelope, providing a stabilising composition…
The effects of rotation on wave-induced transport in stars: the case of an intermediate-mass star
Q. André, S. Mathis, L. Amard
Internal gravity waves propagate in stellar radiative zones and transport angular momentum throughout the evolution of stars, shaping the internal rotation pro le of these regions.…
The effects of rotation on wave-induced transport in stars: from weakly to strongly stratified radiative zones
Q. André, S. Mathis, L. Amard
Internal waves propagating in stellar radiative zones can lead to efficient angular momentum transport, that should occur throughout the whole lifetime of stars. They thus play a k…
Towards a better understanding of tidal dissipation at corotation layers in differentially rotating stars and planets
A. Astoul, S. Mathis, C. Baruteau +1
Star-planet tidal interactions play a significant role in the dynamical evolution of close-in planetary systems. We investigate the propagation and dissipation of tidal inertial wa…
On the orbital evolution of a pair of giant planets in mean motion resonance
Q. André, J. C. B. Papaloizou
Pairs of extrasolar giant planets in a mean motion commensurability are common with 2:1 resonance occurring most frequently. Disc-planet interaction provides a mechanism for their…