Matched filtering of gravitational waves from inspiraling compact binaries: Computational cost and template placement
Benjamin J. Owen (1), B. S. Sathyaprakash (1, 2) ((1) Caltech,, (2) Cardiff)

TL;DR
This paper estimates the computational resources and template placement strategies needed for matched filtering searches of gravitational waves from inspiraling compact binaries across various detectors and configurations.
Contribution
It provides detailed estimates of templates, computational power, and storage requirements for gravitational wave searches using second post-Newtonian waveforms, serving as benchmarks for future methods.
Findings
Initial LIGO requires about 10^11 flops for data analysis.
VIRGO needs approximately 5*10^12 flops, and TAMA requires 1.5*10^11 real numbers for storage.
Advanced LIGO will need around 8*10^11 flops for data processing.
Abstract
We estimate the number of templates, computational power, and storage required for a one-step matched filtering search for gravitational waves from inspiraling compact binaries. These estimates should serve as benchmarks for the evaluation of more sophisticated strategies such as hierarchical searches. We use waveform templates based on the second post-Newtonian approximation for binaries composed of nonspinning compact bodies in circular orbits. We present estimates for six noise curves: LIGO (three configurations), VIRGO, GEO600, and TAMA. To search for binaries with components more massive than 0.2M_o while losing no more than 10% of events due to coarseness of template spacing, initial LIGO will require about 1*10^11 flops (floating point operations per second) for data analysis to keep up with data acquisition. This is several times higher than estimated in previous work by Owen,…
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