Einstein telescope site selection: Seismic and gravity gradient noise
Gravity gradient noise generated by seismic displacements may be the limiting factor for the sensitivity of third-generation gravitational wave detectors at frequencies below 10 Hz. A finite element framework has been developed to calculate the soil response to various excitations. The accompanying gravity gradients as a result of the seismic displacement field can then be evaluated. The results of the gravity gradient noise are in good agreement with previous analytical results. Finally...[Show more]
|Collections||ANU Research Publications|
|Source:||Journal of Physics: Conference Series 203|
|01_van den Brand_Einstein_telescope_site_2010.pdf||815.11 kB||Adobe PDF||Request a copy|
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