Showing 1–20 of 42 results
/ Date/ Name
May 3, 2008SPH Simulations of Direct Impact Accretion in the Ultracompact AM CVn BinariesJan 9, 2012Near-Infrared and X-ray Quasi-Periodic Oscillations in Numerical Models of Sgr A*Oct 18, 2012Dimensional Dependence of the Hydrodynamics of Core-Collapse SupernovaeMar 24, 2014Two-Dimensional Core-Collapse Supernova Models with Multi-Dimensional TransportSep 3, 2009grmonty: a Monte Carlo Code for Relativistic Radiative TransportSep 9, 2019The Overarching Framework of Core-Collapse Supernova Explosions as Revealed by 3D Fornax SimulationsOct 11, 2024Phoebus: Performance Portable GRRMHD for Relativistic AstrophysicsFeb 3, 2026A Method for Thermal Radiation Transport Using Backward Characteristic TracingAug 28, 2006A Hard-to-Soft State Transition during A Luminosity Decline of Aquila X-1Sep 13, 2018A Successful 3D Core-Collapse Supernova Explosion ModelJun 19, 2017A Detailed Comparison of Multi-Dimensional Boltzmann Neutrino Transport Methods in Core-Collapse SupernovaeJan 24, 2018Revival of the Fittest: Exploding Core-Collapse Supernovae from 12 to 25 M$_{\odot}$Sep 24, 2025Characterizing Adaptive Mesh Refinement on Heterogeneous Platforms with Parthenon-VIBENov 20, 2025Asymptotic-preserving semi-implicit finite volume scheme for Extended MagnetohydrodynamicsMar 13, 2012A New Monte Carlo Method for Time-Dependent Neutrino Radiation TransportJul 28, 2015An Integral Condition for Core-Collapse Supernova ExplosionsAug 6, 2018Two-Temperature GRRMHD Simulations of M87Jun 19, 2018Fornax: a Flexible Code for Multiphysics Astrophysical SimulationsFeb 23, 2022PATOKA: Simulating Electromagnetic Observables of Black Hole AccretionFeb 24, 2022Parthenon -- a performance portable block-structured adaptive mesh refinement framework