Beker, M.G.; Cella, G.; DeSalvo, R.; Doets, M.; Grote, Hartmut; Harms, J.; Hennes, E.; Mandic, V.; Rabeling, D.S.; van den Brand, J.F.J.; van Leeuwen, C.M.
(Heidelberg : Springer Verlag, 2011)
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 ...