High Accuracy Gravitational Waveforms from Black Hole Binary Inspirals Using OpenCL
Justin McKennon, Gary Forrester, Gaurav Khanna

TL;DR
This paper introduces a GPU-accelerated, high-accuracy Teukolsky EMRI waveform generator using OpenCL, demonstrating significant performance and scalability improvements for modeling gravitational waves from black hole binaries.
Contribution
The paper presents a novel OpenCL-based implementation of a Teukolsky EMRI code optimized for modern many-core architectures, achieving high accuracy and scalability for gravitational waveform modeling.
Findings
Achieves high-accuracy EMRI waveforms using GPU acceleration.
Demonstrates excellent performance and scalability on supercomputers.
Shows effective utilization of OpenCL across multiple hardware architectures.
Abstract
There is a strong need for high-accuracy and efficient modeling of extreme-mass-ratio binary black hole systems because these are strong sources of gravitational waves that would be detected by future observatories. In this article, we present sample results from our Teukolsky EMRI code: a time-domain Teukolsky equation solver (a linear, hyperbolic, partial differential equation solver using finite-differencing), that takes advantage of several mathematical and computational enhancements to efficiently generate long-duration and high-accuracy EMRI waveforms. We emphasize here the computational advances made in the context of this code. Currently there is considerable interest in making use of many-core processor architectures, such as Nvidia and AMD graphics processing units (GPUs) for scientific computing. Our code uses the Open Computing Language (OpenCL) for taking advantage of the…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Black Holes and Theoretical Physics
