
TL;DR
This paper demonstrates that for gravitational-wave searches, the most effective template bank maximizes detection probability by minimizing a specific mismatch functional, rather than simply minimizing the covering radius, and introduces the concept of an optimal quantizer.
Contribution
It introduces a new criterion for template bank design based on minimizing a mismatch functional, leading to more effective detection strategies than traditional minimum thickness banks.
Findings
Minimizing the mismatch functional G improves detection rates.
Optimal quantizer-based banks outperform minimum thickness banks.
Cubic lattice templates are nearly as effective as more complex lattices.
Abstract
When searching for new gravitational-wave or electromagnetic sources, the signal parameters (masses, sky location, frequencies,...) are unknown. In practice, one hunts for signals at a discrete set of points in parameter space, with a computational cost that is proportional to the number of these points. If that is fixed, the question arises, where should the points be placed in parameter space? The current literature advocates selecting the set of points (called a "template bank") whose Wigner-Seitz (also called Vorono\"i) cells have the smallest covering radius ( smallest maximal mismatch). Mathematically, such a template bank is said to have "minimum thickness". Here, for realistic populations of signal sources, we compute the fraction of potential detections which are "lost" because the template bank is discrete. We show that at fixed computational cost, the minimum…
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