Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities
Bruce Allen, Joseph D. Romano

TL;DR
This paper develops optimal signal processing methods for detecting a stochastic gravitational wave background with laser interferometers, analyzing sensitivities, noise issues, and combining data from multiple detectors.
Contribution
It derives expressions for optimal filters and SNR, and discusses strategies for handling nonstationary noise and multiple detectors in stochastic background searches.
Findings
Derived optimal filter functions and SNR expressions.
Calculated sensitivity levels for various interferometers.
Analyzed data combination strategies for multiple detectors.
Abstract
We analyze the signal processing required for the optimal detection of a stochastic background of gravitational radiation using laser interferometric detectors. Starting with basic assumptions about the statistical properties of a stochastic gravity-wave background, we derive expressions for the optimal filter function and signal-to-noise ratio for the cross-correlation of the outputs of two gravity-wave detectors. Sensitivity levels required for detection are then calculated. Issues related to: (i) calculating the signal-to-noise ratio for arbitrarily large stochastic backgrounds, (ii) performing the data analysis in the presence of nonstationary detector noise, (iii) combining data from multiple detector pairs to increase the sensitivity of a stochastic background search, (iv) correlating the outputs of 4 or more detectors, and (v) allowing for the possibility of correlated noise in…
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