
arXiv: 2409.10383
Abstract We present the numerical relativity module within AthenaK, an open-source performance-portable astrophysics code designed for exascale computing applications. This module employs the Z4c formulation to solve the Einstein equations. We demonstrate its accuracy through a series of standard numerical relativity tests, including convergence of the gravitational waveform from binary black hole coalescence. Furthermore, we conduct scaling tests on OLCF Frontier, NERSC Perlmutter, and ALCF Aurora, where AthenaK exhibits excellent weak-scaling efficiency of 80% on up to 65,536 AMD MI250X GPUs on Frontier (relative to four GPUs) and 67% on Aurora up to 24,576 Intel Data Center Max Series GPUs (relative to 12 GPUs) and strong-scaling efficiencies of 84% and 77% on AMD MI250X and NVIDIA A100 GPUs on Frontier and Perlmutter, respectively. Additionally, we observe a significant performance boost, with 2 orders of magnitude speedup (≳200×) on a GPU compared to a single CPU core, affirming that AthenaK is well suited for exascale computing, and thereby expanding the potential for breakthroughs in numerical relativity research.
Gravitational wave sources, QB460-466, High Energy Astrophysical Phenomena (astro-ph.HE), Black holes, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Compact objects, Instrumentation and Methods for Astrophysics (astro-ph.IM), General Relativity and Quantum Cosmology, Gravitational waves
Gravitational wave sources, QB460-466, High Energy Astrophysical Phenomena (astro-ph.HE), Black holes, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Compact objects, Instrumentation and Methods for Astrophysics (astro-ph.IM), General Relativity and Quantum Cosmology, Gravitational waves
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