Correlation analysis of stochastic gravitational wave background around 0.1-1Hz
General Relativity and Quantum Cosmology
2009-11-11 v3 Astrophysics
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.
Keywords
Cite
@article{arxiv.gr-qc/0510067,
title = {Correlation analysis of stochastic gravitational wave background around 0.1-1Hz},
author = {Naoki Seto},
journal= {arXiv preprint arXiv:gr-qc/0510067},
year = {2009}
}
Comments
11 pages, 7 figures, revised version, to appear in PRD