GR hydro simulation finds that strongly relativistic TDEs evolve like weakly relativistic ones, with persistent eccentric debris, early but short-lived shocks, and slow circularization driven by stream self-interactions.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.HE 3verdicts
UNVERDICTED 3representative citing papers
High-resolution GRMHD simulations show that tearing of tilted accretion disks around rapidly spinning supermassive black holes drives order-of-magnitude variability in continuum and broad-line luminosities on months-to-years timescales, explaining changing-look AGN.
Simulations show magnetic field configurations set truncation radii and resonant cavities that produce QPO frequencies in thin disks matching black hole X-ray binary observations.
citing papers explorer
-
Unexpectedly Weak General Relativistic Effects in Strongly Relativistic Tidal Disruption Events
GR hydro simulation finds that strongly relativistic TDEs evolve like weakly relativistic ones, with persistent eccentric debris, early but short-lived shocks, and slow circularization driven by stream self-interactions.
-
Magnetic Configuration Imprints on Quasi-Periodic Variability in GRMHD Simulations of Thin Accretion Disks
Simulations show magnetic field configurations set truncation radii and resonant cavities that produce QPO frequencies in thin disks matching black hole X-ray binary observations.