Physics
Scientific paper
Mar 1973
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973natur.242..105h&link_type=abstract
Nature, Volume 242, Issue 5393, pp. 105-107 (1973).
Physics
15
Scientific paper
WEBER1-3 has reported detecting pulses of gravitational radiation. The flux density per event is about 3 × 105 erg cm-2 s-1 Hz-1 at 1,660 Hz, implying a possible release of 1054 erg, equivalent to about 1 Msolar, if the radiation originates in the region of the Galactic centre. It has been suggested that if only 1 part in 1025 of the energy were radiated in the electromagnetic spectrum, this could be detected. Some attempts have been made at radio wavelengths4-6, at optical wavelengths (J. T. Delaney, B. Lawless and G. A. Baird, unpublished) and in the X-ray band7,8, but so far without success. Here we describe the results of a new experiment to correlate radio pulses at 858 MHz with events observed by Weber, but to a better radio sensitivity than has been achieved so far. The results are inconclusive at present, but there is strong evidence for the existence of discrete radio pulses of extra-terrestrial origin.
Hughes V. A.
Retallack D. S.
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