Roland Haas

Publications

• Magnetized Outflows from Short-lived Neutron Star Merger Remnants Can Produce a Blue Kilonova
• Addition of tabulated equation of state and neutrino leakage support to illinoisgrmhd
• Numerical relativity higher order gravitational waveforms of eccentric, spinning, nonprecessing binary black hole mergers
• HPC-driven computational reproducibility in numerical relativity codes: a use case study with IllinoisGRMHD
• CarpetX
• CarpetX
• Solving the Bethe-Salpeter equation on massively parallel architectures
• The Einstein Toolkit
• The Einstein Toolkit
• Outflows from Short-Lived Neutron-Star Merger Remnants Can Produce a Blue Kilonova
• HPC-driven computational reproducibility
• APACE: AlphaFold2 and advanced computing as a service for accelerated discovery in biophysics
• A new moment-based general-relativistic neutrino-radiation transport code: Methods and first applications to neutron star mergers
• Deep Learning for Multi-Messenger Astrophysics: A Gateway for Discovery in the Big Data Era
• General relativistic simulations of collapsing binary neutron star mergers with Monte Carlo neutrino transport
• DataVault: A data storage infrastructure for the Einstein toolkit
• Deep learning with quantized neural networks for gravitational wave forecasting of eccentric compact binary coalescence
• Initial data and eccentricity reduction toolkit for binary black hole numerical relativity waveforms
• Source term method for binary neutron stars initial data
• Initial data and eccentricity reduction toolkit for binary black hole numerical relativity waveforms
• GRaM-X: A new GPU-accelerated dynamical spacetime GRMHD code for Exascale computing with the Einstein Toolkit
• General relativistic simulations of collapsing binary neutron star mergers with Monte-Carlo neutrino transport
• Numerical relativity higher order gravitational waveforms of eccentric, spinning, non-precessing binary black hole mergers
• The Einstein Toolkit
• The Einstein Toolkit
• The Einstein Toolkit
• The Einstein Toolkit
• The Einstein Toolkit
• The Einstein Toolkit
• GRaM-X: a new GPU-accelerated dynamical spacetime GRMHD code for Exascale computing with the Einstein Toolkit
• The Einstein Toolkit
• Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter
• A magnetar engine for short GRBs and kilonovae
• Solving the Bethe-Salpeter equation on massively parallel architectures
• Multipolar effective-one-body waveforms for precessing binary black holes: Construction and validation
• Observation of eccentric binary black hole mergers with second and third generation gravitational wave detector networks
• A Magnetar Engine for Short GRBs and Kilonovae
• Unequal mass binary neutron star simulations with neutrino transport: Ejecta and neutrino emission
• Multipolar effective-one-body waveforms for precessing binary black holes: Construction and validation
• Observation of eccentric binary black hole mergers with second and third generation gravitational wave detector networks
• DataVault: a data storage infrastructure for the Einstein Toolkit
• Source term method for binary neutron stars initial data
• Physics of eccentric binary black hole mergers: A numerical relativity perspective
• Deep Learning with Quantized Neural Networks for Gravitational Wave Forecasting of Eccentric Compact Binary Coalescence
• IllinoisGRMHD: GRMHD code for dynamical spacetimes
• Enabling real-time multi-messenger astrophysics discoveries with deep learning
• Fusing numerical relativity and deep learning to detect higher-order multipole waveforms from eccentric binary black hole mergers
• Deep Learning with Quantized Neural Networks for Gravitational-wave Forecasting of Eccentric Compact Binary Coalescence
• General Relativistic Stability and Gravitational Wave Content of Rotating Triaxial Neutron Stars
• APACE: AlphaFold2 and advanced computing as a service for accelerated discovery in biophysics
• POWER: Python Open-source Waveform ExtractoR
• Evolution of the Magnetized, Neutrino-Cooled Accretion Disk in the Aftermath of a Black Hole Neutron Star Binary Merger
• Supporting high-performance and high-throughput computing for experimental science
• Container solutions for HPC Systems: A Case Study of Using Shifter on BlueWaters
• BOSS-LDG: A novel computational framework that brings together Blue Waters, Open Science Grid, Shifter and the LIGO Data Grid to accelerate gravitational wave discovery
• Python open source waveform ExtractoR (POWER): An open source, Python package to monitor and post-process numerical relativity simulations
• Gravitational Waves from Binary Black Hole Mergers Inside of Stars
• Supporting High-Performance and High-Throughput Computing for Experimental Science
• The nanograv 11-year data set: Pulsar-Timing constraints on the stochastic gravitational-Wave background
• Enabling real-time multi-messenger astrophysics discoveries with deep learning
• Unequal mass binary neutron star simulations with neutrino transport: Ejecta and neutrino emission
• Deep learning for multi-messenger astrophysics a gateway for discovery in the big data era
• Time-symmetry, symplecticity and stability of Euler-Maclaurin and Lanczos-Dyche integration
• Physics of eccentric binary black hole mergers: A numerical relativity perspective
• Gravitational waveforms from SpEC simulations: neutron star-neutron star and low-mass black hole-neutron star binaries
• Fusing numerical relativity and deep learning to detect higher-order multipole waveforms from eccentric binary black hole mergers
• R-process nucleosynthesis from three-dimensional magnetorotational core-collapse supernovae
• THE PROGENITOR DEPENDENCE OF THREE-DIMENSIONAL CORE-COLLAPSE SUPERNOVAE
• Eccentric, nonspinning, inspiral Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers
• Evolution of the Magnetized, Neutrino-Cooled Accretion Disk in the Aftermath of a Black Hole Neutron Star Binary Merger
• BOSS-LDG: A novel computational framework that brings together blue waters, open science grid, shifter and the LIGO data grid to accelerate gravitational wave discovery
• The Presync project: Synchronization automation in the cactus framework
• Container solutions for HPC systems: A case study of using shifter on blue waters
• r-process Nucleosynthesis from Three-dimensional Magnetorotational Core-collapse Supernovae
• Improved Analysis of GW150914 Using a Fully Spin-Precessing Waveform Model
• Gravitational waveforms from spectral Einstein code simulations: Neutron star-neutron star and low-mass black hole-neutron star binaries
• Simulations of inspiraling and merging double neutron stars using the Spectral Einstein Code
• Time-symmetry, symplecticity and stability of Euler-Maclaurin and Lanczos-Dyche integration
• The NCSA eccentric gravitational waveform catalog
• Supporting High-Performance and High-Throughput Computing for Experimental Science
• Container solutions for HPC Systems: A Case Study of Using Shifter on Blue Waters
• The NANOGrav 11 Year Data Set: Pulsar-timing Constraints on the Stochastic Gravitational-wave Background
• Evolution of the magnetized, neutrino-cooled accretion disk in the aftermath of a black hole-neutron star binary merger
• The Progenitor Dependence of Core-collapse Supernovae from Three-dimensional Simulations with Progenitor Models of 12-40 M ⊙
• Eccentric, nonspinning, inspiral, Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers
• Python Open source Waveform ExtractoR (POWER): an open source, Python package to monitor and post-process numerical relativity simulations
• Detection and characterization of eccentric compact binary coalescence at the interface of numerical relativity, analytical relativity and machine learning
• BOSS-LDG using Blue Waters for LIGO data analysis
• Evolution of the Magnetized, Neutrino-Cooled Accretion Disk in the Aftermath of a Black Hole Neutron Star Binary Merger
• Assessing confidence in numerical relativity waveforms of binary neutron star mergers
• Influence of higher-order waveform multipoles for the detection of eccentric binary black hole mergers
• Numerical Relativity Simulations of Compact Binary Populations in Dense Stellar Environments
• Gravitational Waves from Binary Black Hole Mergers inside Stars
• BOSS-LDG: A Novel Computational Framework that Brings Together Blue Waters, Open Science Grid, Shifter and the LIGO Data Grid to Accelerate Gravitational Wave Discovery
• Complete waveform model for compact binaries on eccentric orbits
• Development of accurate waveform models for eccentric compact binaries with numerical relativity simulations
• General-Relativistic Three-Dimensional Multi-group Neutrino Radiation-Hydrodynamics Simulations of Core-Collapse Supernovae
• Erratum: Binary neutron stars with arbitrary spins in numerical relativity [Phys. Rev. D 92, 124012 (2015)]
• Observing gravitational-wave transient GW150914 with minimal assumptions
• Gravitational waveforms for neutron star binaries from binary black hole simulations
• Low mass binary neutron star mergers: Gravitational waves and neutrino emission
• Binary neutron stars with arbitrary spins in numerical relativity
• Binary NS simulations using SpEC
• General relativistic magneto-hydrodynamics with the Einstein Toolkit
• The Einstein Toolkit: a community computational infrastructure for relativistic astrophysics
• Neutrino-driven Convection and SASI in Three-Dimensional Core-Collapse Supernovae
• Mode-sum regularization of the scalar self-force: Formulation in terms of a tetrad decomposition of the singular field
• Correlated gravitational wave and neutrino signals from general-relativistic rapidly rotating iron core collapse
• Tidal Disruptions of White Dwarfs from Ultra-close Encounters with Intermediate-mass Spinning Black Holes
• Constructing better initial data for compact binary systems
• Error-analysis and comparison to analytical models of numerical waveforms produced by the NRAR Collaboration
• Three-dimensional general-relativistic hydrodynamic simulations of binary neutron star coalescence and stellar collapse with multipatch grids
• Self-force as a cosmic censor
• GRHydro: a new open-source general-relativistic magnetohydrodynamics code for the Einstein toolkit
• Neutrino-driven Convection in Core-collapse Supernovae: High-resolution Simulations
• Gravitational waveforms for neutron star binaries from binary black hole simulations
• A large-scale dynamo and magnetoturbulence in rapidly rotating core-collapse supernovae
• IllinoisGRMHD: an open-source, user-friendly GRMHD code for dynamical spacetimes
• Neutrino-driven Turbulent Convection and Standing Accretion Shock Instability in Three-dimensional Core-collapse Supernovae
• Post-merger evolution of a neutron star-black hole binary with neutrino transport
• Neutron star-black hole mergers with a nuclear equation of state and neutrino cooling: Dependence in the binary parameters
• Magnetorotational Core-collapse Supernovae in Three Dimensions
• The Magnetorotational Explosion Mechanism in Full 3D Core-Collapse Supernova Simulations
• Formation and Coalescence of Cosmological Supermassive-Black-Hole Binaries in Supermassive-Star Collapse
• Scalar self-force for eccentric orbits around a Schwarzschild black hole
• GRB060218 as a Tidal Disruption of a White Dwarf by an Intermediate-mass Black Hole
• General-relativistic Simulations of Three-dimensional Core-collapse Supernovae
• A New Channel for Low-Luminosity GRBs: Tidal Disruptions of White Dwarfs by Intermediate Mass Black Holes
• Three-Dimensional General Relativistic Simulations of Core-Collapse Supernovae
• The Gravitational-Wave Signature of Core-Collapse Supernovae
• Binary NS simulations using SpEC
• Tidal disruption of white dwarfs by intermediate mass black holes
• Prompt emission from tidal disruptions of white dwarfs by intermediate mass black holes
• Late inspiral and merger of binary black holes in scalar-tensor theories of gravity
• Late Inspiral and Merger of Binary Black Holes in Scalar-Tensor Theories of Gravity
• Binary NS simulations using SpEC
• Mergers of Supermassive Black Holes in Astrophysical Environments
• Time domain calculation of the electromagnetic self-force on eccentric geodesics in Schwarzschild spacetime
• Properties of accretion flows around coalescing supermassive black holes
• Flares from Disruptions of White Dwarfs by Intermediate Mass Black Holes
• Gravitational and Electromagnetic Signatures from the Tidal Disruption of a White Dwarf by an Intermediate Mass Black Hole
• Electromagnetic Emission from the Last Hours of Merging Supermassive Black Holes
• General initial data for simulations of compact binary systems
• Relativistic Mergers of Supermassive Black Holes and Their Electromagnetic Signatures
• Gravitational and Electromagnetic Signatures from the Tidal Disruption of a White Dwarf by an Intermediate Mass Black Hole
• Binary Black Hole Mergers in a Gas Cloud and their Electromagnetic Signatures
• Black Hole - Neutron Star Binary Simulations at Georgia Tech
• Self-force on point particles in orbit around a Schwarzschild black hole
• Scalar self-force on eccentric geodesics in Schwarzschild spacetime: A time-domain computation
• Mass change and motion of a scalar charge in cosmological spacetimes
• Updating the SPP Benchmark Suite for Extreme-Scale Systems
• Benchmarking Parallelized File Aggregation Tools for Large Scale Data Management
• Efficient Software for Archiving and Retrieving Results of Massive Bioinformatics Analyses in High-Performance Computing Environments
• AsterX: a new open-source GPU-accelerated GRMHD code for dynamical spacetimes
• AI-driven Conservative-to-Primitive Conversion in Hybrid Piecewise Polytropic and Tabulated Equations of State
• Phase Stability in the 3-Dimensional Open-source Code for the Chiral mean-field Model
• SciCode: A Research Coding Benchmark Curated by Scientists
• Waveform Modelling for the Laser Interferometer Space Antenna
• Einstein Toolkit
• 3D full-GR simulations of magnetorotational core-collapse supernovae on GPUs: A systematic study of rotation rates and magnetic fields
• DataVault: A data storage infrastructure for the Einstein Toolkit