The long-term evolution of a black hole accretion torus: a comparison between GRMHD simulations and relativistic thin disk theory
astro-ph.HE
Submitted: 2026-10-26
Updated: 2026-10-26
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