Astronomy and Astrophysics – Astronomy
Scientific paper
May 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.199..659m&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 199, May 1982, p. 659-666. Research supported by the Deutsche Forschung
Astronomy and Astrophysics
Astronomy
21
Background Radiation, Electromagnetic Noise, Gravitational Waves, Pulsars, Spectral Energy Distribution, Stochastic Processes, Coherent Radiation, Electromagnetic Pulses, Energy Spectra, Time Measurement, Wave Propagation
Scientific paper
The influence of a stochastic and isotropic background of gravitational radiation on timing measurements of pulsars is investigated, and it is shown that pulsar timing noise may be used to establish a significant upper limit of about 10 to the -10th on the total energy density of very long-wavelength stochastic gravitational waves. This places restriction on the strength of very long wavelength gravitational waves in the Friedmann model, and such a background is expected to have no significant effect on the approximately 3 K electromagnetic background radiation or on the dynamics of a cluster of galaxies.
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