Weakly modeled search for compact binary coalescences in the Einstein Telescope
Adrian Macquet, Tito Dal Canton, Tania Regimbau

TL;DR
This paper evaluates a computationally efficient, weakly modeled search algorithm for detecting gravitational waves from compact binary coalescences in the Einstein Telescope data, highlighting its effectiveness and background estimation method.
Contribution
It demonstrates that a weakly modeled search can recover a significant fraction of CBC signals in ET data, offering a less sensitive but more computationally feasible alternative to matched filtering.
Findings
Recovered 38% of binary black hole mergers
Recovered 89% of high-mass systems (above 100 solar masses)
Estimated BNS chirp mass with 1.3% precision
Abstract
We search for gravitational-wave (GW) signals from compact binary coalescences (CBC) in the mock data challenge of the Einstein Telescope (ET) with a detection algorithm that does not rely on the waveform of the signal searched. With the increased sensitivity of ET compared to current GW detectors, a very high rate of detectable sources is expected in the data, and the computational cost of the searches may become a limiting factor. This is why we explore the behavior of a weakly modeled search algorithm, which is intrinsically less sensitive than optimal search methods based on matched filtering techniques, but computationally much cheaper. This search recovers a significant fraction of CBC signals present in the data: 38% of the total number of binary black hole mergers, including 89% of the systems with a total mass above 100 solar masses, as well as the majority of binary…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Gamma-ray bursts and supernovae · Scientific Research and Discoveries
