Chasing 5-sigma: Prospects for searches for long-duration gravitational-waves without time slides

TL;DR

This paper introduces an analytic background estimation method for seedless clustering in gravitational-wave searches, reducing computational costs and improving detection prospects for long-duration signals.

Contribution

It presents a novel analytic approach to estimate background noise in seedless clustering, enhancing efficiency for long-duration gravitational-wave transient searches.

Findings

Analytic background model agrees qualitatively with Monte Carlo and real data.

The method can supplement traditional background estimation techniques.

Potential to improve sensitivity and reduce computational costs in gravitational-wave searches.

Abstract

The detection of unmodeled gravitational-wave bursts by ground-based interferometric gravitational-wave detectors is a major goal for the advanced detector era. These searches are commonly cast as pattern recognition problems, where the goal is to identify statistically significant clusters in spectrograms of strain power when the precise signal morphology is unknown. In previous work, we have introduced a clustering algorithm referred to as "seedless clustering," and shown that it is a powerful tool for detecting weak long-lived (10-1000s) signals in background. However, as the algorithm is currently conceived, in order to carry out an all-sky search on a $\approx$ year of data, significant computational resources may be required in order to carry out background estimation. Alternatively, some of the sensitivity of the search must be sacrificed to control computational costs. The sensitivity of the algorithm is limited by the amount of computing resources due to the requirement of performing background studies to assign significance in gravitational-wave searches. In this paper, we present an analytic method for estimating the background generated by the seedless clustering algorithm and compare the performance to both Monte Carlo Gaussian noise and time-shifted gravitational-wave data from a week of LIGO's 5th Science Run. We demonstrate qualitative agreement between the model and measured distributions and argue that the approximation will be useful to supplement conventional background estimation techniques for advanced detector searches for long-duration gravitational-wave transients.