The Implications of the Microwave Background Anisotropies for Laser-Interferometer-Tested Gravitational Waves
L. P. Grishchuk
TL;DR
This paper discusses how microwave background anisotropies and quantum cosmological perturbations suggest the existence of detectable relic gravitational waves within the frequency ranges of LISA and ground-based interferometers.
Contribution
It links microwave background anisotropies with the potential detection of relic gravitational waves by laser interferometers, highlighting their measurable implications.
Findings
Relic gravitational waves are predicted to be detectable by LISA and ground-based interferometers.
Quantum-generated cosmological perturbations imply a measurable gravitational wave background.
Microwave background anisotropies provide constraints on gravitational wave amplitudes.
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.
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