An upper limit on the stochastic background of ultralow-frequency gravitational waves

Details An upper limit on the stochastic background of ultralow-frequency gravitational waves An upper limit on the stochastic background of ultralow-frequency gravitational waves

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...265l..35r&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 265, Feb. 15, 1983, p. L35-L37.

Mathematics

50

Background Radiation, Cosmology, Gravitational Waves, Pulsars, Stochastic Processes, Time Measurement, Closure Law, Extremely Low Radio Frequencies, Gravitation Theory, Limits (Mathematics), Power Spectra, Relativity, Spectral Energy Distribution

Scientific paper

Using pulse arrival time data for PSR 1237+25, a pulsar with unusually regular timing behavior, the authors place a firm upper limit on the magnitude of any stochastic background of low-frequency gravitational radiation in the universe. At frequencies between 0.3×10-8 and 3×10-8 Hz, the equivalent energy density limits are well below those needed to close the universe on account of gravitational waves alone.

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