activity
20242026
collaborators

6 papers

astro-ph.HE2026

Complex dynamical regimes of the Tayler-Spruit dynamo

Paul Barrère, Jérôme Guilet, Basile Gallet +1

Astrophysical dynamos feature various spatial structures and dynamical regimes, ranging from hemispherical magnetic fields to the random reversals of the geodynamo. The recently ob…

astro-ph.SR2026

Coexisting Tayler instability-driven dynamos in radiative zones: New dynamo solution and its impacts on stellar physics

Paul Barrère, Alexis Reboul-Salze, Patrick Eggenberger +4

Recent asteroseismic observations constitute a great challenge for rotating stellar evolution models, which predict overly fast internal rotation rates when only hydrodynamic proce…

astro-ph.HE2025

From proto-neutron star dynamo to low-field magnetars

Andrei Igoshev, Paul Barrère, Raphaël Raynaud +3

Low-field magnetars have dipolar magnetic fields that are 10-100 times weaker than the threshold, G, used to define classical magnetars, yet they produce simila…

astro-ph.HE2024

Tayler-Spruit dynamo in binary neutron star merger remnants

Alexis Reboul-Salze, Paul Barrère, Kenta Kiuchi +4

In binary neutron star mergers, the remnant can be stabilized by differential rotation before it collapses into a black hole. Therefore, the angular momentum transport mechanisms a…

astro-ph.HE2024

Tayler-Spruit dynamo in stably stratified rotating fluids: Application to proto-magnetars

Paul Barrère, Jérôme Guilet, Raphaël Raynaud +1

The formation of highly magnetized young neutron stars, called magnetars, is still a strongly debated question. A promising scenario invokes the amplification of the magnetic field…

astro-ph.SR2024

Observational characterisation of large-scale transport and horizontal turbulent diffusivity in the quiet Sun

F. Rincon, P. Barrère, T. Roudier

The Sun is a magnetic star, and the only spatio-temporally resolved astrophysical system displaying turbulent MHD thermal convection. This makes it a privileged object of study to…