The Implications of the Microwave Background Anisotropies for Laser-Interferometer-Tested Gravitational Waves
arXiv:gr-qc/9609062 · doi:10.1088/0264-9381/14/6/009
Abstract
The observed microwave background anisotropies in combination with the theory of quantum mechanically generated cosmological perturbations predict a well measurable amount of relic gravitational waves in the frequency intervals tested by LISA and ground-based laser interferometers.
revised, corrected, and slightly expanded version to be published in Classical and Quantum Gravity; 22 pages, 1 Postscript figure, Latex; Based on a talk presented at the First Internationsl LISA Symposium, 9 - 12 July 1996, RAL, UK
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