The International Gravitational Event Collaboration (IGEC) involves a network of five cryogenic resonant-cylinder gravity-wave detectors: two in Italy and one each in Switzerland, the US, and Australia. The search for passing gravity waves is a delicate art; in the resonant-cylinder approach, it means measuring strain displacements far smaller than the size of an atomic nucleus on the end faces of 3-meter-long, 2000-kg metal cylinders. The IGEC team has now reported that in its first operational period, covering 1997 and 1998, no gravity waves were detected. From this they calculated an annual upper limit of four events with a mean Fourier component exceeding 10−20 Hz−1 arriving at Earth. The IGEC typically used thresholds that correspond to the conversion of 0.04–0.11 solar masses to gravity waves in an astrophysical source…such as a coalescing binary system of neutron stars or black holes…at the Galactic center. The collaboration also demonstrated that a...
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1 January 2001
January 01 2001
New upper limit on gravity-wave events Available to Purchase
Philip F. Schewe
Physics Today 54 (1), 9 (2001);
Citation
Philip F. Schewe; New upper limit on gravity-wave events. Physics Today 1 January 2001; 54 (1): 9. https://doi.org/10.1063/1.4796215
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