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

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

2005-10-14

arxiv.org/abs/gr-qc/0510067v3

Phys.Rev. D73 (2006) 063001

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

11 pages, 7 figures, revised version, to appear in PRD

Scientific paper

10.1103/PhysRevD.73.063001

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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