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Einstein telescope site selection: Seismic and gravity gradient noise

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dc.contributor.authorVan Den Brand, J.
dc.contributor.authorBeker, M G
dc.contributor.authorDoets, M
dc.contributor.authorHennes, E.
dc.contributor.authorRabeling, David
dc.coverage.spatialRome Italy
dc.date.accessioned2015-12-13T22:29:04Z
dc.date.createdJuly 1-5 2009
dc.date.issued2010
dc.date.updated2016-02-24T10:06:07Z
dc.description.abstractGravity 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 results of gravity gradient noise from a single pulse excitation of a homogenous medium are discussed for an underground detector.
dc.identifier.urihttp://hdl.handle.net/1885/74512
dc.publisherIOP Publishing
dc.relation.ispartofseriesEleventh International Conference on Topics in Astroparticle and Underground Physics (TAUP) 2009
dc.sourceJournal of Physics: Conference Series 203
dc.source.urihttp://iopscience.iop.org/1742-6596/203/1
dc.subjectKeywords: Analytical results; Finite Element; Gravitational wave detectors; Gravity gradients; Limiting factors; Seismic displacement; Single-pulse excitations; Soil response; Third generation; Underground detectors; Seismology; Site selection
dc.titleEinstein telescope site selection: Seismic and gravity gradient noise
dc.typeConference paper
local.bibliographicCitation.lastpage3
local.bibliographicCitation.startpage1
local.contributor.affiliationvan den Brand, J F J, Nikhef, National Institute for Subatomic Physics
local.contributor.affiliationBeker, M G, Nikhef
local.contributor.affiliationDoets, M, National Institute for Subatomic
local.contributor.affiliationHennes, E., Nikhef Amsterdam
local.contributor.affiliationRabeling, David, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidRabeling, David, u4074112
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020102 - Astronomical and Space Instrumentation
local.identifier.ariespublicationU3488905xPUB4161
local.identifier.doi10.1088/1742-6596/203/1/012076
local.identifier.scopusID2-s2.0-77950485798
local.type.statusPublished Version

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