activity
20232026
most citedFORGE'd in FIRE II: The Formation of Magnetically-Dominated Quasar Accretion Disks from Cosmological Initial Conditions

49 citations · 115 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2026

Explaining the X-ray Precursor, Ultra-long Prompt Emission, and Week-long Decay of GRB250702B with a Jetted Micro-TDE

Fulya Kıroğlu, Taeho Ryu, Alexander Tchekhovskoy +3

The longest detected gamma-ray burst, GRB250702B, exhibited seven hours of prompt -ray emission, preceded by a soft X-ray precursor ( day earlier) and followed by a weeks…

astro-ph.HE2026★ 3 cited

Thick Disks, Thin Hopes: Suppressed Capture and Merger Rates in AGN

Yashvardhan Tomar, Philip F. Hopkins, Kyle Kremer

Multiple models have been suggested over the years to explain the structure and support of accretion disks around supermassive black holes, from the standard thin thermal-pressure-…

astro-ph.GA2025

Connecting Cores and Black Hole Dynamics Across Scales: From Globular Clusters to Massive Ellipticals

Kyle Kremer, Newlin C. Weatherford, Philip F. Hopkins +2

The centers of massive elliptical galaxies exhibit a wide range in density profiles, from central cusps to resolved cores with order kiloparsec sizes. The cored ellipticals have be…

astro-ph.HE2025

Compact Objects in Globular Clusters

Kyle Kremer

It is now widely established that globular clusters host robust populations of white dwarfs, neutron stars, and black holes throughout their lifetimes. Within clusters, dynamical p…

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.GA2024★ 16 cited

From Seeds to Supermassive Black Holes: Capture, Growth, Migration, and Pairing in Dense Proto-Bulge Environments

Yanlong Shi, Kyle Kremer, Philip F. Hopkins

The origins and mergers of supermassive black holes (BHs) remain a mystery. We describe a scenario from a novel multi-physics simulation featuring rapid (Myr) hyper-E…

astro-ph.GA2024★ 8 cited

Feedback-regulated Seed Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei

Yanlong Shi, Kyle Kremer, Philip F. Hopkins

The detection of supermassive black holes (SMBHs) in high-redshift luminous quasars may require a phase of rapid accretion, and as a precondition, substantial gas influx toward see…

astro-ph.GA2024★ 12 cited

FORGE'd in FIRE III: The IMF in Quasar Accretion Disks from STARFORGE

Philip F. Hopkins, Michael Y. Grudic, Kyle Kremer +3

Recently, we demonstrated self-consistent formation of strongly-magnetized quasar accretion disks (QADs) from cosmological radiation-magnetohydrodynamic-thermochemical galaxy-star…

astro-ph.HE2023★ 17 cited

An Analytic Model For Magnetically-Dominated Accretion Disks

Philip F. Hopkins, Jonathan Squire, Eliot Quataert +6

Recent numerical cosmological radiation-magnetohydrodynamic-thermochemical-star formation simulations have resolved the formation of quasar accretion disks with Eddington or super-…

astro-ph.HE2023★ 49 cited

FORGE'd in FIRE II: The Formation of Magnetically-Dominated Quasar Accretion Disks from Cosmological Initial Conditions

Philip F. Hopkins, Jonathan Squire, Kung-Yi Su +9

In a companion paper, we reported the self-consistent formation of quasar accretion disks with inflow rates down to <300 Schwarzschild radii fro…