Greg Bryan

Professor

Columbia University

United States

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Greg Bryan is a Professor at Columbia University, USA. His research focuses on cosmological simulations, with recent articles exploring topics such as the accretion processes onto black holes, the dynamics of stellar wind-blown bubbles, and the influence of the Large Magellanic Cloud on the Milky Way. He employs advanced simulation techniques to investigate the physical principles governing galaxy formation and evolution.

Greg Bryan

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Articles (30)

Field-level Comparison and Robustness Analysis of Cosmological N-body Simulations

Prevention is better than cure? Feedback from high specific energy winds in cosmological simulations with Arkenstone

Simulating high-velocity clouds in the observational plane: an initial study with the Smith Cloud

The Coevolution of Stellar Wind-blown Bubbles and Photoionized Gas. I. Physical Principles and a Semianalytic Model

The Coevolution of Stellar Wind-blown Bubbles and Photoionized Gas. II. 3D RMHD Simulations and Tests of Semianalytic Models

Accretion onto supermassive and intermediate-mass black holes in cosmological simulations

The All-sky Impact of the LMC on the Milky Way Circumgalactic Medium

You Shall Not Pass! The Propagation of Low-/Moderate-powered Jets Through a Turbulent Interstellar Medium

Self-regulation of high-redshift black hole accretion via jets: challenges for SMBH formation

AEOS: Star-by-star Cosmological Simulations of Early Chemical Enrichment and Galaxy Formation

High-spectral-resolution Observations of the Optical Filamentary Nebula Surrounding NGC 1275

Metallicity Dependence of Pressure-regulated Feedback-modulated Star Formation in the TIGRESS-NCR Simulation Suite

Geometry, Dissipation, Cooling, and the Dynamical Evolution of Wind-blown Bubbles

The Structure and Composition of Multiphase Galactic Winds in a Large Magellanic Cloud Mass Simulated Galaxy

Katachi (形): Decoding the Imprints of Past Star Formation on Present-day Morphology in Galaxies with Interpretable CNNs*

Unravelling jet quenching criteria across L* galaxies and massive cluster ellipticals

Observational Predictions for the Survival of Atomic Hydrogen in Simulated Fornax-like Galaxy Clusters

Taming the TuRMoiL: The Temperature Dependence of Turbulence in Cloud–Wind Interactions

When and How Ram Pressure Stripping in Low-mass Satellite Galaxies Enhances Star Formation

Code Comparison in Galaxy-scale Simulations with Resolved Supernova Feedback: Lagrangian versus Eulerian Methods

Active galactic nucleus jet feedback in hydrostatic haloes

Calibrating Cosmological Simulations with Implicit Likelihood Inference Using Galaxy Growth Observables

On the impact of runaway stars on dwarf galaxies with resolved interstellar medium

The Anatomy of a Turbulent Radiative Mixing Layer: Insights from an Analytic Model with Turbulent Conduction and Viscosity

Gas Accretion Can Drive Turbulence in Galaxies

Regulation of Star Formation by a Hot Circumgalactic Medium

Efficient Long-range Active Galactic Nuclei (AGNs) Feedback Affects the Low-redshift Lyα Forest

Self-regulation of black hole accretion via jets in early protogalaxies

An Exploration of AGN and Stellar Feedback Effects in the Intergalactic Medium via the Low-redshift Lyα Forest

If Dark Matter is Fuzzy, the First Stars Form in Massive Pancakes

Collaborators (17)

Rachel Somerville

Christoph Pfrommer

Yuan Li

Romain Teyssier

Mark Krumholz

Laurence Perreault-Levasseur

Megan Donahue

Eve Ostriker

Masayuki Akiyama

Lamiya A. Mowla

Ji-hoon Kim

Volker Springel

Romeel Davé

Lori Porter

Anna Frebel

Laurent Drissen

Jingyao Zhu

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