activity
20232026
most citedMixing is easy: New insights for cosmochemical evolution from pre-stellar core collapse

16 citations · 18 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.EP2026

Revisiting the picture of circumbinary disc truncation

Enrico Ragusa, Elliot Lynch, Guillaume Laibe +1

Circumbinary discs are observed to develop central cavities carved by the gravitational influence of the binary. Analytical estimates of cavity sizes predict truncation at $\sim 2…

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.EP2025

Radial modes of pressure bumps and dips in astrophysical discs

Armand Leclerc, Guillaume Laibe, Elliot Lynch +1

This study investigates the signatures of pressure extrema on global oscillations in discs. To this end, we use the framework of wave topology to establish a generalised local disp…

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.EP2024★ 2 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…

astro-ph.SR2024

Local Spherical Collapsing Box in Athena++: Numerical Implementation and Benchmark Tests

Ziyan Xu, Elliot M. Lynch, Guillaume Laibe

We implement a local model for a spherical collapsing/expanding gas cloud into the Athena++ magnetohydrodynamic code. This local model consists of a Cartesian periodic box with tim…

astro-ph.SR2024

PT and anti-PT symmetries for astrophysical waves

Armand Leclerc, Guillaume Laibe, Nicolas Perez

Context: Discrete symmetries have found numerous applications in photonics and quantum mechanics, but remain little studied in fluid mechanics, particularly in astrophysics. Aims:…

astro-ph.SR2024★ 16 cited

Mixing is easy: New insights for cosmochemical evolution from pre-stellar core collapse

Asmita Bhandare, Benoît Commerçon, Guillaume Laibe +5

Signposts of early planet formation are ubiquitous in substructured young discs. Dense, hot and high-pressure regions formed during gravitational collapse process, integral to star…

physics.flu-dyn2024

Topology of shallow-water waves on the rotating sphere

Nicolas Perez, Armand Leclerc, Guillaume Laibe +1

Topological properties of the spectrum of shallow-water waves on a rotating spherical body are established. Particular attention is paid to its spectral flow, i.e. the modes whose…

astro-ph.SR2023

The Exceptional Ring of buoyancy instability in stars

Armand Leclerc, Lucien Jezequel, Nicolas Perez +3

We reveal properties of global modes of linear buoyancy instability in stars, characterised by the celebrated Schwarzschild criterion, using non-Hermitian topology. We identify a r…