Sensitivity of a VIRGO pair to stochastic GW backgrounds
Danilo Babusci (Laboratori Nazionali di Frascati, INFN) Massimo, Giovannini(Institute for Theoretical Physics, Lausanne University)
TL;DR
This paper evaluates how well a pair of VIRGO detectors can detect stochastic gravitational wave backgrounds, considering different detector overlaps and spectral types, to improve understanding of cosmological GW signals.
Contribution
It provides a detailed analysis of VIRGO pair sensitivity to various cosmological gravitational wave backgrounds, including overlap configurations and spectral models.
Findings
VIRGO pair sensitivity varies with detector overlap.
Detectability of relic GW improves with specific spectral assumptions.
Analysis informs future GW detection strategies.
Abstract
The sensitivity of a pair of VIRGO interferometers to gravitational waves backgrounds (GW) of cosmological origin is analyzed for the cases of maximal and minimal overlap of the two detectors. The improvements in the detectability prospects of scale-invariant and non-scale-invariant logarithmic energy spectra of relic GW are discussed.
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