Kyle Parfrey

The Confrontation between General Relativity and Experiment

THE ROLE OF THE MAGNETOROTATIONAL INSTABILITY IN MASSIVE STARS

First results from the IllustrisTNG simulations: matter and galaxy clustering

Plasmoid formation in global GRMHD simulations and AGN flares

Large-scale galaxy bias

Magnetic Reconnection and Hot Spot Formation in Black Hole Accretion Disks

Cosmological tests of general relativity: A principal component analysis

Large-scale structure in brane-induced gravity. II. Numerical simulations

Sgr A* near-infrared flares from reconnection events in a magnetically arrested disc

Non-thermal particle acceleration in collisionless relativistic electron–proton reconnection

Large-scale poloidal magnetic field dynamo leads to powerful jets in GRMHD simulations of black hole accretion with toroidal field

N-body simulations of DGP and degravitation theories

MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS

A parameter survey of Sgr A* radiative models from GRMHD simulations with self-consistent electron heating

Modified gravity and cosmology

First-Principles Plasma Simulations of Black-Hole Jet Launching

Evolution of galaxy bias, generalized

Black hole jets without large-scale net magnetic flux

Particle acceleration in axisymmetric pulsar current sheets

The Origin of Solar Activity in the Tachocline

Scale-dependent halo bias from scale-dependent growth