activity
19972022
most citedEfficient Generation of Jets from Magnetically Arrested Accretion on a Rapidly Spinning Black Hole

1.3k citations · 12.7k across the 67 of their papers we have counts for

collaborators

67 papers

astro-ph.HE2022

PATOKA: Simulating Electromagnetic Observables of Black Hole Accretion

George N. Wong, Ben S. Prather, Vedant Dhruv +11

The Event Horizon Telescope (EHT) has released analyses of reconstructed images of horizon-scale millimeter emission near the supermassive black hole at the center of the M87 galax…

astro-ph.HE2019★ 343 cited

The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project

Oliver Porth, Koushik Chatterjee, Ramesh Narayan +25

Recent developments in compact object astrophysics, especially the discovery of merging neutron stars by LIGO, the imaging of the black hole in M87 by the Event Horizon Telescope (…

astro-ph.HE2018★ 362 cited

A unified model for tidal disruption events

Lixin Dai, Jonathan C. McKinney, Nathaniel Roth +2

In the past few years wide-field optical and UV transient surveys as well as X-ray telescopes have allowed us to identify a few dozen candidate tidal disruption events (TDEs). Whil…

astro-ph.HE2017★ 10 cited

Observational Signatures of Mass-Loading in Jets Launched by Rotating Black Holes

Michael O' Riordan, Asaf Pe'er, Jonathan C. McKinney

It is widely believed that relativistic jets in X-ray binaries and active-galactic nuclei are powered by the rotational energy of black holes. This idea is supported by general-rel…

astro-ph.HE2017★ 39 cited

Angular Momentum Transport in Thin Magnetically Arrested Disks

Megan D. Marshall, Mark J. Avara, Jonathan C. McKinney

In accretion disks with large-scale ordered magnetic fields, the magnetorotational instability (MRI) is marginally suppressed, so other processes may drive angular momentum transpo…

astro-ph.HE2017★ 35 cited

General Relativistic Radiation Magnetohydrodynamic Simulations of Thin Magnetically Arrested Disks

Danilo Morales Teixeira, Mark J. Avara, Jonathan C. McKinney

The classical, relativistic thin-disk theory of Novikov and Thorne (NT) predicts a maximum accretion efficiency of 40% for an optically thick, radiatively efficient accretion disk…