Beker, M G; Cella, G; DeSalvo, R; Doets, M; Grote, H; Harms, J.; Hennes, E.; Mandic, V.; Rabeling, David; Van Den Brand, J.; van Leeuwen, J
The next generation gravitational wave interferometric detectors will likely be underground detectors to extend the GW detection frequency band to frequencies below the Newtonian noise limit. Newtonian noise originates from the continuous motion of the Earth's crust driven by human activity, tidal stresses and seismic motion, and from mass density fluctuations in the atmosphere. It is calculated that on Earth's surface, on a typical day, it will exceed the expected GW signals at frequencies...[Show more]
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