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Correlation analysis of stochastic gravitational wave background around 0.1-1Hz

Naoki Seto
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Abstract

We discuss prospects for direct measurement of stochastic gravitational wave background around 0.1-1Hz with future space missions. It is assumed to use correlation analysis technique with the optimal TDI variables for two sets of LISA-type interferometers. The signal to noise for detection of the background and the estimation errors for its basic parameters (amplitude, spectral index) are evaluated for proposed missions.

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Naoki Seto. 2006-01-20. Correlation analysis of stochastic gravitational wave background around 0.1-1Hz. https://doi.org/10.1103/physrevd.73.063001

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