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Observation of Gravitational Waves from a Binary Black Hole Merger
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February 2016 |
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GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
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October 2017 |
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Exploring the sensitivity of next generation gravitational wave detectors
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January 2017 |
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Cosmos++ : Relativistic Magnetohydrodynamics on Unstructured Grids with Local Adaptive Refinement
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December 2005 |
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Numerical 3+1 General Relativistic Magnetohydrodynamics: A Local Characteristic Approach
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January 2006 |
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Total Variation Diminishing Scheme for Relativistic Magnetohydrodynamics
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January 2001 |
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Numerical {3 + 1} General Relativistic Hydrodynamics: A Local Characteristic Approach
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February 1997 |
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A Second-Order Godunov Method for Multi-Dimensional Relativistic Magnetohydrodynamics
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January 2011 |
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Adaptive mesh refinement for hyperbolic partial differential equations
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March 1984 |
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Constraint violation in free evolution schemes: Comparing the BSSNOK formulation with a conformal decomposition of the Z4 formulation
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April 2010 |
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Tidal effects in binary neutron star coalescence
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August 2012 |
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Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms
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May 2012 |
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A finite element method for angular discretization of the radiation transport equation on spherical geodesic grids
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October 2023 |
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An improved weighted essentially non-oscillatory scheme for hyperbolic conservation laws
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March 2008 |
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High-accuracy numerical simulation of black-hole binaries: Computation of the gravitational-wave energy flux and comparisons with post-Newtonian approximants
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November 2008 |
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Solving 3D relativistic hydrodynamical problems with weighted essentially nonoscillatory discontinuous Galerkin methods
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October 2016 |
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A high-order finite volume method for systems of conservation laws—Multi-dimensional Optimal Order Detection (MOOD)
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May 2011 |
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GRChombo : Numerical relativity with adaptive mesh refinement
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December 2015 |
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A limiter for PPM that preserves accuracy at smooth extrema
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July 2008 |
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The Piecewise Parabolic Method (PPM) for gas-dynamical simulations
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April 1984 |
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Energy Versus Angular Momentum in Black Hole Binaries
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March 2012 |
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GR-Athena++: Puncture Evolutions on Vertex-centered Oct-tree Adaptive Mesh Refinement
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November 2021 |
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ECHO: a Eulerian conservative high-order scheme for general relativistic magnetohydrodynamics and magnetodynamics
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July 2007 |
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A positivity-preserving adaptive-order finite-difference scheme for GRMHD
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November 2023 |
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Flux-corrected transport techniques for multidimensional compressible magnetohydrodynamics
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January 1991 |
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On Godunov-type methods near low densities
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February 1991 |
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Quantifying uncertainties in general relativistic magnetohydrodynamic codes
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May 2023 |
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IllinoisGRMHD: an open-source, user-friendly GRMHD code for dynamical spacetimes
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August 2015 |
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Massively Parallel Simulations of Binary Black Hole Intermediate-Mass-Ratio Inspirals
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January 2019 |
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Massively parallel simulations of binary black holes with adaptive wavelet multiresolution
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March 2023 |
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Relativistic fluid disks in orbit around Kerr black holes
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July 1976 |
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Implementation of Monte Carlo Transport in the General Relativistic SpEC Code
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October 2021 |
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Numerical Simulations of Optically Thick Accretion onto a Black Hole. i. Spherical case
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June 2012 |
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Numerical Simulations of Optically Thick Accretion onto a Black Hole. ii. Rotating flow
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October 2014 |
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Waveform systematics in the gravitational-wave inference of tidal parameters and equation of state from binary neutron-star signals
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June 2021 |
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HARM: A Numerical Scheme for General Relativistic Magnetohydrodynamics
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May 2003 |
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An unsplit Godunov method for ideal MHD via constrained transport
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May 2005 |
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An unsplit Godunov method for ideal MHD via constrained transport in three dimensions
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April 2008 |
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The exact solution of the Riemann problem in relativistic magnetohydrodynamics
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August 2006 |
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WhiskyMHD: a new numerical code for general relativistic magnetohydrodynamics
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June 2007 |
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Can magnetic fields be detected during the inspiral of binary neutron stars?
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October 2009 |
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High Order Strong Stability Preserving Time Discretizations
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September 2008 |
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Parthenon—a performance portable block-structured adaptive mesh refinement framework
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December 2022 |
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On Upstream Differencing and Godunov-Type Schemes for Hyperbolic Conservation Laws
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January 1983 |
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Compact binary evolutions with the Z4c formulation
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October 2013 |
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Pseudospectral method for gravitational wave collapse
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March 2016 |
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Distinguishing the nature of comparable-mass neutron star binary systems with multimessenger observations: GW170817 case study
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September 2019 |
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Gravitational Waves from Inspiraling Compact Binaries with Magnetic Dipole Moments
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July 2000 |
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Global high-order numerical schemes for the time evolution of the general relativistic radiation magneto-hydrodynamics equations
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June 2023 |
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AsterX: a new open-source GPU-accelerated GRMHD code for dynamical spacetimes
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December 2024 |
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Robust recovery of primitive variables in relativistic ideal magnetohydrodynamics
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January 2021 |
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SpECTRE: A task-based discontinuous Galerkin code for relativistic astrophysics
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April 2017 |
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Implementation of advanced Riemann solvers in a neutrino-radiation magnetohydrodynamics code in numerical relativity and its application to a binary neutron star merger
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December 2022 |
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A splitting method for numerical relativistic magnetohydrodynamics
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November 2024 |
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A Godunov-type scheme for relativistic magnetohydrodynamics
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February 1999 |
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First Order Quasilinear Equations in Several Independent Variables
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February 1970 |
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Relativistic MHD simulations of extragalactic jets
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May 2005 |
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Dissipation and Heating in Supersonic Hydrodynamic and mhd Turbulence
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February 2009 |
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The Einstein Toolkit: a community computational infrastructure for relativistic astrophysics
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May 2012 |
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Science case for the Einstein telescope
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March 2020 |
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A Measurement of the Electromagnetic Luminosity of a Kerr Black Hole
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August 2004 |
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An HLLC Riemann solver for relativistic flows – II. Magnetohydrodynamics
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April 2006 |
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Beyond second-order convergence in simulations of magnetized binary neutron stars with realistic microphysics
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October 2019 |
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Type II critical phenomena of neutron star collapse
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September 2008 |
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Primitive Variable Solvers for Conservative General Relativistic Magnetohydrodynamics
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April 2006 |
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Direct Calculation of the Radiative Efficiency of an Accretion disk Around a Black hole
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February 2009 |
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Velocity-induced collapses of stable neutron stars
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September 2001 |
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Large eddy simulations of magnetized mergers of neutron stars with neutrinos
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May 2022 |
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Effects of the microphysical equation of state in the mergers of magnetized neutron stars with neutrino cooling
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August 2015 |
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An operator-splitting numerical scheme for relativistic magnetohydrodynamics
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April 2024 |
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High accuracy binary black hole simulations with an extended wave zone
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February 2011 |
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The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project
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August 2019 |
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The black hole accretion code
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May 2017 |
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Increasing the accuracy of binary neutron star simulations with an improved vacuum treatment
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November 2020 |
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Gravitational waveform accuracy requirements for future ground-based detectors
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May 2020 |
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Lessons for adaptive mesh refinement in numerical relativity
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June 2022 |
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A new moment-based general-relativistic neutrino-radiation transport code: Methods and first applications to neutron star mergers
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March 2022 |
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GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations
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journal
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January 2018 |
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THC: a new high-order finite-difference high-resolution shock-capturing code for special-relativistic hydrodynamics
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October 2012 |
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High-order fully general-relativistic hydrodynamics: new approaches and tests
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March 2014 |
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Beyond second-order convergence in simulations of binary neutron stars in full general relativity
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October 2013 |
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High-Order Numerical-Relativity Simulations of Binary Neutron Stars
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preprint
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January 2015 |
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Adaptive mesh refinement in binary black holes simulations
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April 2024 |
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Formation and Coalescence of Cosmological Supermassive-Black-Hole Binaries in Supermassive-Star Collapse
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October 2013 |
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GW170817, general relativistic magnetohydrodynamic simulations, and the neutron star maximum mass
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January 2018 |
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Numerical simulations of super-critical black hole accretion flows in general relativity
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January 2014 |
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Semi-implicit scheme for treating radiation under M1 closure in general relativistic conservative fluid dynamics codes
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January 2013 |
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GRaM-X: a new GPU-accelerated dynamical spacetime GRMHD code for Exascale computing with the Einstein Toolkit
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September 2023 |
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Modeling GW170817 based on numerical relativity and its implications
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December 2017 |
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Non-linear pulsations in differentially rotating neutron stars: mass-shedding-induced damping and splitting of the fundamental mode
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August 2004 |
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The Athena++ Adaptive Mesh Refinement Framework: Design and Magnetohydrodynamic Solvers
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June 2020 |
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The new discontinuous Galerkin methods based numerical relativity program Nmesh
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December 2022 |
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Kokkos 3: Programming Model Extensions for the Exascale Era
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January 2021 |
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Towards the ultimate conservative difference scheme. II. Monotonicity and conservation combined in a second-order scheme
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March 1974 |
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Quasi-radial modes of rotating stars in general relativity
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April 2001 |
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Solving the relativistic magnetohydrodynamics equations with ADER discontinuous Galerkin methods, a posteriori subcell limiting and adaptive mesh refinement
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July 2015 |
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Binary neutron star merger simulations with neutrino transport and turbulent viscosity: impact of different schemes and grid resolution
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January 2023 |