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- W1532560311 abstract "The Laser Interferometer Gravitational-waveObservatory (LIGO) attempts to detect ripples in the curvature ofspacetime using two large scale interferometers. These detectorsare several kilometer long Michelson interferometers withFabry-Perot cavities between two silica test masses in each arm.Given Earth's proximity to various astrophysical phenomena LIGOmust be sensitive to relative displacements of 1018 m and thusrequires multiple levels of noise reduction to ensure the isolationof the interferometer components from numerous sources of noise. Asubstantial contributor to the Advanced LIGO noise in the 1-10 Hzrange is Newtonian (or gravity gradient) noise which arises fromlocal fluctuations in the Earth's gravitational field. Densityfluctuations from seismic activity as well as acoustic andturbulent phenomenon in the Earth's atmosphere both contribute toslight variations in the local value of g. Given the directcoupling of gravitational fields to mass the LIGO test massescannot be shielded from this noise. In an attempt to characterizeand reduce Newtonian noise in interferometric gravitational wavedetectors we investigate seismic and atmospheric contributions tothe noise and consider the effect of submerging a gravitationalwave detector." @default.
- W1532560311 created "2016-06-24" @default.
- W1532560311 creator A5068039799 @default.
- W1532560311 date "2011-01-01" @default.
- W1532560311 modified "2023-09-23" @default.
- W1532560311 title "Novel approaches to Newtonian noise suppression in interferometric gravitational wave detection" @default.
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