activity
20242026
most citedDeveloping a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows

2 citations · 2 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026

Rescaling Transforms for Local Models of Spherical Flows

Elliot M. Lynch, Guillaume Laibe

Previously we developed a local model for a spherically contracting/expanding gas cloud that can be used to study turbulence and small scale instabilities in such flows. In this wo…

astro-ph.SR2025

A core-sensitive mixed / mode of the Sun predicted by wave topology and hydrodynamical simulation

Arthur Le Saux, Armand Leclerc, Guillaume Laibe +2

Helioseismology has revolutionized our understanding of the Sun by analyzing its global oscillation modes. However, the solar core remains elusive, limiting a full understanding of…

astro-ph.SR2025

The importance of Berry phase in solar acoustic modes

Armand Leclerc, Guillaume Laibe

An analytic expression for the frequencies of standing waves in stars, applicable to any radial order n, is derived from ray-tracing equations by the mean of Wigner-Weyl calculus.…

astro-ph.EP20242 cited

Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows

Elliot M. Lynch, Guillaume Laibe

In the astrophysics community it is common practice to model collisionless dust, entrained in a gas flow, as a pressureless fluid. However a pressureless fluid is fundamentally dif…

astro-ph.SR2024

Wave topology of stellar inertial oscillations

Armand Leclerc, Guillaume Laibe, Nicolas Perez

Inertial waves in convective regions of stars exhibit topological properties linked to a Chern number of 1. The first of these is a unique, unidirectional, prograde oscillation mod…