Hamiltonian variational reconstruction of the 3D magnetic geometry of relativistic jets: accuracy across GRMHD models and the fundamental sign degeneracy
astro-ph.HE
Submitted: 2026-07-10
Updated: 2026-09-05
Comments: 14 pages, 13 figures, 4 tables
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Related papers
- Accreting Neutron Stars in Low-Mass X-ray Binaries
- Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
- Early panchromatic spectra reveal helium in the thermonuclear supernova 2024kce
- Multiwavelength Classification of Chandra Sources in Omega Centauri
- Impact of the equation of state on core collapse supernovae I: the low- T/W instability
- Secular Evolution of Quasiperiodic Eruptions: eRO-QPE2