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Wide band detectors for gravitational waves
Gravitational wave interferometric detectors operating between 10 Hz and 10 kHz are currently being built. According to current astrophysical knowledge their sensitivity - of the order of 10-23 m/Hz at 100 Hz - should allow to detect a few events per year. The expected signals include binary neutron...
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| Lenguaje: | eng eng |
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CERN
1997
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| Acceso en línea: | http://cds.cern.ch/record/423809 |