activity
20182026
most citedH-AMR: A New GPU-accelerated GRMHD Code for Exascale Computing With 3D Adaptive Mesh Refinement and Local Adaptive Time-stepping

102 citations · 465 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.GA2026

Balmer Absorption Series and Broad Metal Lines in Two Luminous Little Red Dots

Bingjie Wang, Jenny E. Greene, Hanpu Liu +21

Balmer absorption is common among little red dots (LRDs), but absorbers at or redward of systemic are rare, occurring in only \% of H absorbers. In this paper, we stu…

astro-ph.HE2026

Little Red Dots As Super-Eddington Fountain Flows

Nicholas Kaaz, Eliot Quataert, Taya Govreen-Segal +1

Little red dots (LRDs) may be powered by supermassive black holes (SMBHs) accreting above the Eddington limit. Spectroscopy of LRDs often shows absorption troughs blueshifted by $\…

astro-ph.HE2025

Changing-Look AGN Powered By Disk Tearing

Nicholas Kaaz, Matthew Liska, Charlotte Ward +1

Changing-look active galactic nuclei (CLAGN) feature order-of-magnitude variability in both the continuum and broad line luminosities on months-to-years long timescales, and are cu…

astro-ph.GA2025★ 10 cited

Zooming In On The Multi-Phase Structure of Magnetically-Dominated Quasar Disks: Radiation From Torus to ISCO Across Accretion Rates

Philip F. Hopkins, Kung-Yi Su, Norman Murray +12

Recent radiation-thermochemical-magnetohydrodynamic simulations resolved formation of quasar accretion disks from cosmological scales down to ~300 gravitational radii , argu…

astro-ph.HE2024★ 20 cited

H-AMR FORGE'd in FIRE I: Magnetic state transitions, jet launching and radiative emission in super-Eddington, highly magnetized quasar disks formed from cosmological initial conditions

Nicholas Kaaz, Matthew Liska, Alexander Tchekhovskoy +2

Quasars are powered by supermassive black hole (SMBH) accretion disks, yet standard disk models are inconsistent with many quasar observations. Recently, Hopkins et al. (2024) simu…

astro-ph.HE2024★ 4 cited

Extreme scale height variations and nozzle shocks in warped disks

Nicholas Kaaz, Yoram Lithwick, Matthew Liska +1

Accretion disks around both stellar-mass and supermassive black holes are likely often warped. Whenever a disk is warped, its scale height varies with azimuth. Sufficiently strong…