Abstract
THE gravitational radiation received by Weber1 at a frequency ν= 1,660 Hz, over a bandwidth Δω≈0.1, had pulse durations < 0.4 s and an average pulse frequency f ≈ 10−5.5 s−1 (that is, about one in four days). The energy (in the pseudo-tensor approximation) in each pulse must have been ∼ 104 ergs cm−2 over the bandwidth. If a flat spectrum is assumed up to ω≈104 s−1 (cutoff somewhere beyond this value) the total energy per cm2 in a pulse must be F Δt > 109 erg cm−2. The average energy density is then F Δt· f/c > 10−7 erg cm−3, and the corresponding mass density ρg > 10−28 g cm−3.
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References
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Hénon, M., Astron. Astrophys., 2, 151 (1969).
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KAFKA, P. “Gravars”. Nature 226, 436–439 (1970). https://doi.org/10.1038/226436a0
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DOI: https://doi.org/10.1038/226436a0
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