MG13 - Talk detail |
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Participant |
van den Brand, Johannes | |||||||
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Institution |
Nikhef - Science Park 105 - Amsterdam - NH - Netherland | |||||||
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Session |
GW4 |
Accepted |
No |
Order |
5 |
Time |
16:30 - 16:55 | 25' |
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Talk |
Oral abstract |
Title |
Seismic noise and subtraction of gravity gradient noise | |||||
| Co-authors | Mark Beker | |||||||
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Abstract |
Fluctuations of the local gravitational field as a result of seismic and atmospheric displacements will limit the sensitivity of ground based gravitational wave detectors at frequencies below 10 Hz. We discuss the implications of Newtonian noise for future third generation gravitational wave detectors. The relevant seismic wave fields are predominately of human origin and are dependent on local infrastructure and population density. Results from seismic studies will be presented that show that considerable seismic noise reduction is possible compared to current detector locations. A realistic seismic amplitude spectral density of a suitably quiet site should not exceed 0.5 nm/rtHz (Hz/f)**2 above 1 Hz. Newtonian noise models have been developed both analytically and by finite element analysis. These show that the contribution to Newtonian noise from surface waves due to distance sources significantly reduces with depth. Seismic displacements from local sources and body waves then become the dominant contributors to the Newtonian fluctuations. |
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