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Conference Paper

Low-frequency sources of gravitational waves

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Schutz,  Bernard F.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Citation

Schutz, B. F. (1993). Low-frequency sources of gravitational waves. In M. Demianski, & C. W. F. Everitt (Eds.), The first William Fairbank Meeting on Relativistic Gravitational Experiments in Space: proceedings of the meeting held at the University of Rome, September 10 - 14, 1990. Singapore [u.a.]: World Scientific.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0013-752D-2
Abstract
Future space-based gravitational wave detectors may have a frequency range extending down to 10-4Hz. Many interesting sources are likely to be detected in this range: the formation of large-mass black holes, close binary systems of compact objects and of normal stars, and a cosmological background of radiation that may contain the signature of the earliest directly observed events in the Universe.