activity
20162026
most citedLayered semi-convection and tides in giant planet interiors - II. Tidal dissipation

16 citations · 29 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2026★ 1 cited

Multi-epoch afterglow rebrightenings in GRB 250129A: Evidence for successive shock interactions

D. Akl, S. Antier, H. Koehn +105

Most long gamma-ray bursts (GRBs) exhibit afterglows broadly consistent with external forward-shock emission, typically described by smooth broken power-law decays in the multiband…

astro-ph.EP2019★ 16 cited

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…

astro-ph.SR2019

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.…

astro-ph.SR2018

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…

astro-ph.SR2017

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…

astro-ph.EP2017

Layered semi-convection and tides in giant planet interiors - I. Propagation of internal waves

Quentin André, Adrian J. Barker, Stéphane Mathis

Layered semi-convection is a possible candidate to explain Saturn's luminosity excess and the abnormally large radius of some hot Jupiters. In giant planet interiors, it could lead…