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20052026
most citedRadiative Models of Sgr A* from GRMHD Simulations

317 citations · 3.1k across the 42 of their papers we have counts for

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Showing astro-ph.HEShow all

21 papers · 1 filter

astro-ph.HE2024

Phoebus: Performance Portable GRRMHD for Relativistic Astrophysics

Brandon Barker, Mariam Gogilashvili, Janiris Rodriguez-Bueno +6

We introduce the open source code PHOEBUS (phifty one ergs blows up a star) for astrophysical general relativistic radiation magnetohydrodynamic simulations. PHOEBUS is designed fo…

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.HE2021★ 48 cited

Iharm3D: Vectorized General Relativistic Magnetohydrodynamics

Cora Prather, George N. Wong, Vedant Dhruv +4

Iharm3D is an open-source C code for simulating black hole accretion systems in arbitrary stationary spacetimes using ideal general-relativistic magnetohydrodynamics (GRMHD). It is…

astro-ph.HE2019★ 85 cited

Full Transport General Relativistic Radiation Magnetohydrodynamics for Nucleosynthesis in Collapsars

Jonah M. Miller, Trevor M. Sprouse, Christopher L. Fryer +4

We model a compact black hole-accretion disk system in the collapsar scenario with full transport, frequency dependent, general relativistic radiation magnetohydrodynamics. We exam…

astro-ph.HE2019★ 280 cited

The Overarching Framework of Core-Collapse Supernova Explosions as Revealed by 3D Fornax Simulations

Adam Burrows, David Radice, David Vartanyan +3

We have conducted nineteen state-of-the-art 3D core-collapse supernova simulations spanning a broad range of progenitor masses. This is the largest collection of sophisticated 3D s…

astro-ph.HE2019★ 21 cited

MOCMC: Method of Characteristics Moment Closure, a Numerical Method for Covariant Radiation Magnetohydrodynamics

Benjamin R. Ryan, Joshua C. Dolence

We present a conservative numerical method for radiation magnetohydrodynamics with frequency-dependent full transport in stationary spacetimes. This method is stable and accurate f…