activity
20202026
most citedNumerical simulations of the Tayler-Spruit dynamo in proto-magnetars

20 citations · 56 across the 12 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2026

A first-principles binary neutron star merger model of GW170817, GRB170817A, and AT2017gfo

Kenta Kiuchi, Sho Fujibayashi, Kota Hayashi +6

The multimessenger observation of the binary neutron star merger event GW170817, associated with its electromagnetic counterparts GRB170817A and AT2017gfo, marked a milestone in as…

astro-ph.HE2026

A magnetar formation in binary neutron star merger

Kenta Kiuchi, Alexis Reboul-Salze, Yuichiro Sekiguchi +1

We conduct a global general relativistic neutrino-radiation-transfer magnetohydrodynamics simulation of a - binary neutron star with the unprecedented spatial re…

astro-ph.HE2026★ 1 cited

Probing millisecond magnetar formation in binary neutron star mergers through X-ray follow-up of gravitational wave alerts

Clara Plasse, Alexis Reboul-Salze, Jérome Guilet +5

The nature of the remnant of a binary neutron star (BNS) merger is uncertain. Though certainly a black hole (BH) in the cases of the most massive BNSs, X-ray lightcurves from gamma…

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 +3

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★ 1 cited

Non-linear saturation of gravito-inertial modes excited by tidal resonances in binary neutron stars

Alexis Reboul-Salze, Aurélie Astoul, Hao-Jui Kuan +1

During the last seconds of a binary neutron-star merger, the tidal force can excite stellar oscillation modes to large amplitudes. From the perspective of premerger electromagnetic…

astro-ph.HE2025★ 1 cited

MRI-driven dynamo at high Pm numbers

Alexis Reboul-Salze, Loren E. Held, Kenta Kiuchi

To power gamma-ray bursts and other high-energy events, large-scale magnetic fields are required to extract rotational energy from compact objects such as black holes and neutron s…