activity
20082026
most citedEfficiency of Thin Magnetically-Arrested Disks Around Black Holes

97 citations · 545 across the 16 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2026

Spin Demographics of Active Supermassive Black Holes: Updated Estimates from X-ray reflection and Future opportunities

Julia M. Sisk-Reynes, Christopher S. Reynolds, James H. Matthews +5

Understanding the growth of supermassive black holes (SMBHs) requires observational constraints on how their angular momentum (or spin) varies with mass, since the relative importa…

astro-ph.HE2025★ 1 cited

Non-Equilibrium Thermodynamics of Black-Hole Coronae: QPOs, Turbulence, and Jets

Vanessa López-Barquero, Alejandro Jenkins, Christopher S. Reynolds +1

The variability of X-rays observed from accreting black hole systems, including quasi-periodic oscillations (QPOs), suggests a complex nonlinear dynamics in the corona. Here, we pr…

astro-ph.HE2025★ 1 cited

Evidence for Supermassive Black Hole Binaries

Martin G. H. Krause, Martin A. Bourne, Silke Britzen +10

We review the state of the evidence for the existence and observational appearance of supermassive black hole binaries. Such objects are expected from standard hierarchical galaxy…

astro-ph.HE2025

Disk warping and black hole X-ray binaries I. Tentative unification of low-frequency quasi-periodic oscillations

Gregoire Marcel, Samuel Turner, Benjamin Ricketts +6

X-ray binaries exhibit complex variability patterns studied in the power-spectrum. These include the broad-band noise (BBN) components and various types of narrow components called…

astro-ph.HE2018★ 33 cited

The influence of accretion disk thickness on the large-scale magnetic dynamo

J. Drew Hogg, Christopher Reynolds

The evolution of the magnetic field from the large-scale dynamo is considered a central feature of the accretion disk around a black hole. The resulting low-frequency oscillations…

astro-ph.HE2018★ 22 cited

The Dynamics of Truncated Black Hole Accretion Disks II: Magnetohydrodynamic Case

J. Drew Hogg, Christopher S. Reynolds

We study a truncated accretion disk using a well-resolved, semi-global magnetohydrodynamic simulation that is evolved for many dynamical times (6096 inner disk orbits). The spectra…