Detecting a stochastic background of gravitational waves by correlating n detectors

Abstract

We discuss the optimal detection strategy for a stochastic background of gravitational waves in the case n detectors are available. In literature so far, only two cases have been considered: 2- and n-point correlators. We generalize these analysises to m-point correlators (with m<n) built out of the n detector signals, obtaining the result that the optimal choice is to combine 2-point correlators. Correlating n detectors in this optimal way will improve the (suitably defined) signal-to-noise ratio with respect to the n=2 case by a factor equal to the fourth root of n(n-1)/2. Finally we give an estimation of how this could improve the sensitivity for a network of multi-mode spherical antennas.

arXiv comment12 pages, version accepted by Class. & Quant. Grav

References in corpus (4)

• Gravitational Wave Experiments and Early Universe Cosmology
• Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities
• Gravitational radiation from cosmic (super)strings: bursts, stochastic background, and observational windows
• Stochastic background of gravitational waves generated by a cosmological population of young, rapidly rotating neutron stars

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