Pulsar timing and upper limits on a cosmic background of gravitational waves

Details Pulsar timing and upper limits on a cosmic background of gravitational waves Pulsar timing and upper limits on a cosmic background of gravitational waves

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.249...84m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 249, March 1, 1991, p. 84-90. DFG-supported research.

Statistics

Computation

5

Background Radiation, Cosmic Rays, Gravitational Waves, Pulsars, Computational Astrophysics, Probability Distribution Functions, Stochastic Processes

Scientific paper

The zero-frequency limit of the spectrum of a stochastic background of gravitational waves is discussed. The influence of the low-frequency end of the background spectrum on the timing noise of pulsars can be described in terms of an effective random walk of the pulsar along the earth-pulsar direction. The possibility of observing this random walk in pulsar timing residuals is briefly explored.

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