activity
20242026
collaborators

8 papers

astro-ph.HE2026

Jets from Scratch: Dynamo-Generated Poloidal Magnetic Fields in 3D Collapsar Simulations

Ho-Sang Chan, Ore Gottlieb, Jonatan Jacquemin-Ide +2

The origin of the large-scale poloidal magnetic field required to power relativistic jets in collapsars remains uncertain. While such a field may be inherited during PNS collapse,…

astro-ph.HE2026

Evidence for Low Universal Equilibrium Black Hole Spin in Luminous Magnetically Arrested Disks

Beverly Lowell, Jonatan Jacquemin-Ide, Matthew Liska +1

Relativistic collimated outflows, or jets, provide a crucial mode of active galactic nucleus feedback. Although jets extract their energy from the black hole (BH) rotation, their e…

astro-ph.HE2025

Demystifying flux eruptions: Magnetic flux transport in magnetically arrested disks

Jonatan Jacquemin-Ide, Mitchell C. Begelman, Beverly Lowell +3

Magnetically arrested disks (MADs) are a compelling model for explaining variability in low-luminosity active galactic nuclei (AGN), including horizon-scale outbursts like those ob…

astro-ph.HE2025

Magnetically-Driven Neutron-Rich Ejecta Unleashed: Global 3D Neutrino-General Relativistic Magnetohydrodynamic Simulations of Collapsars Probe the Conditions for r-process Nucleosynthesis

Danat Issa, Ore Gottlieb, Brian Metzger +5

Collapsars - rapidly rotating stellar cores that form black holes - can power gamma-ray bursts (GRBs) and are proposed to be key contributors to the production of heavy elements in…

astro-ph.HE2025

Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling

Pedro Naethe Motta, Jonatan Jacquemin-Ide, Rodrigo Nemmen +2

X-ray binaries (XRBs) display spectral state transitions that are accompanied by substantial changes in the hardness, luminosity, and structure of the accretion flow. We developed…

astro-ph.HE2025

Black Hole Spin-down in Collapsars in 3D Neutrino Transport GRMHD Simulations

Danat Issa, Beverly Lowell, Jonatan Jacquemin-Ide +2

Collapsars -- massive stars whose cores promptly collapse into black holes (BHs) -- can power long-duration gamma-ray bursts (LGRBs) via relativistic, collimated, electromagnetical…