TL;DR
This paper introduces a scalable computational framework for simulating binary black hole inspirals with high mass ratios, aiding gravitational wave research and astrophysics.
Contribution
It presents a novel, highly scalable adaptive mesh framework combining octree and wavelet methods for simulating intermediate-mass-ratio black hole mergers.
Findings
Achieved excellent weak scalability up to 131,000 cores.
Successfully simulated binary mergers with mass ratios up to 100.
Generated waveforms for LIGO data analysis.
Abstract
We present a highly-scalable framework that targets problems of interest to the numerical relativity and broader astrophysics communities. This framework combines a parallel octree-refined adaptive mesh with a wavelet adaptive multiresolution and a physics module to solve the Einstein equations of general relativity in the BSSN formulation. The goal of this work is to perform advanced, massively parallel numerical simulations of Intermediate Mass Ratio Inspirals (IMRIs) of binary black holes with mass ratios on the order of 100:1. These studies will be used to generate waveforms as used in LIGO data analysis and to calibrate semi-analytical approximate methods. Our framework consists of a distributed memory octree-based adaptive meshing framework in conjunction with a node-local code generator. The code generator makes our code portable across different architectures. The equations…
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