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High Accuracy Gravitational Waveforms from Black Hole Binary Inspirals Using OpenCL
General Relativity and Quantum Cosmology · Submitted 1 Jun 2012
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We present the performance of our Teukolsky EMRI code on multiple modern processor architectures and demonstrate the high level of accuracy and performance it is able to achieve.
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The abstract, sentence by sentence
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 massive parallelism offered by modern GPU architectures. We present the performance of our Teukolsky EMRI code on multiple modern processor architectures and demonstrate the high level of accuracy and performance it is able to achieve. We also present the code's scaling performance on a large supercomputer i.e. NSF's XSEDE resource: Keeneland (a 201 TeraFLOP/s, 120-node HP SL390 system with 240 Intel Xeon 5660 CPUs and 360 NVIDIA Fermi M2070 graphics processors, with the nodes connected by an InfiniBand QDR network).
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | 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. | background 1.00 | 0.05 | 0.05 | asserted 1.00 |
| s1 | 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. | contribution 0.93 | 0.93 | 0.22 | asserted 0.99 |
| s2 | We emphasize here the computational advances made in the context of this code. | contribution 0.89 | 0.35 | 0.04 | asserted 0.58 |
| s3 | 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. | background 1.00 | 0.04 | 0.02 | asserted 0.98 |
| s4 | Our code uses the Open Computing Language (OpenCL) for taking advantage of the massive parallelism offered by modern GPU architectures. | method 0.94 | 0.87 | 0.06 | asserted 1.00 |
| s5 | We present the performance of our Teukolsky EMRI code on multiple modern processor architectures and demonstrate the high level of accuracy and performance it is able to achieve. | contribution 0.63 | 0.96 | 0.50 | asserted 1.00 |
| s6 | We also present the code's scaling performance on a large supercomputer i.e. NSF's XSEDE resource: Keeneland (a 201 TeraFLOP/s, 120-node HP SL390 system with 240 Intel Xeon 5660 CPUs and 360 NVIDIA Fermi M2070 graphics processors, with the nodes connected by an InfiniBand QDR network). | contribution 0.47 | 0.93 | 0.09 | asserted 0.99 |
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The paper
Original 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 massive parallelism offered by modern GPU architectures. We present the performance of our Teukolsky EMRI code on multiple modern processor architectures and demonstrate the high level of accuracy and performance it is able to achieve. We also present the code's scaling performance on a large supercomputer i.e. NSF's XSEDE resource: Keeneland (a 201 TeraFLOP/s, 120-node HP SL390 system with 240 Intel Xeon 5660 CPUs and 360 NVIDIA Fermi M2070 graphics processors, with the nodes connected by an InfiniBand QDR network).
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References
How the literature uses it
3 arXiv papers cite this in 8 sentences
Papers citing it · 6 sentences without a confident label
Uses its method or tool 2 papers
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Details on this parallel implementation and careful measurements of gains in overall performance can be found in Ref. [ref] .
Small mass plunging into a Kerr black hole: Anatomy of the inspiral-merger-ringdown waveforms · Numerical solution of the time-domain Teukolsky equation · 0.87
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In the time domain, we use an approach similar to that of Refs. [ref] .
Divergences in gravitational-wave emission and absorption from extreme mass ratio binaries · Time and frequency domain integrators · 0.99
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