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Low-frequency terrestrial gravitational-wave detectors

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dc.contributor.authorHarms, Jan
dc.contributor.authorSlagmolen, Bram
dc.contributor.authorAdhikari, Rana
dc.contributor.authorColeman Miller, M
dc.contributor.authorEvans, Matthew
dc.contributor.authorChen, Yanbei
dc.contributor.authorMuller, Holger
dc.contributor.authorAndo, Masaki
dc.date.accessioned2015-12-10T23:04:36Z
dc.date.available2015-12-10T23:04:36Z
dc.date.issued2013
dc.date.updated2015-12-10T08:46:32Z
dc.description.abstractDirect detection of gravitational radiation in the audio band is being pursued with a network of kilometer-scale interferometers (LIGO, Virgo, KAGRA). Several space missions (LISA, DECIGO, BBO) have been proposed to search for sub-hertz radiation from massive astrophysical sources. Here we examine the potential sensitivity of three ground-based detector concepts aimed at radiation in the 0.1-10 Hz band. We describe the plethora of potential astrophysical sources in this band and make estimates for their event rates and thereby, the sensitivity requirements for these detectors. The scientific payoff from measuring astrophysical gravitational waves in this frequency band is great. Although we find no fundamental limits to the detector sensitivity in this band, the remaining technical limits will be extremely challenging to overcome.
dc.identifier.issn1550-7998
dc.identifier.urihttp://hdl.handle.net/1885/62440
dc.publisherAmerican Physical Society
dc.sourcePhysical Review D-Particles, Fields, Gravitation and Cosmology
dc.titleLow-frequency terrestrial gravitational-wave detectors
dc.typeJournal article
local.bibliographicCitation.issue12
local.contributor.affiliationHarms, Jan, INFN
local.contributor.affiliationSlagmolen, Bram, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationAdhikari, Rana, LIGO - California Institute of Technology
local.contributor.affiliationColeman Miller, M, University of Maryland
local.contributor.affiliationEvans, Matthew, Massachusetts Institute of Technology
local.contributor.affiliationChen, Yanbei, California Institute of Technology
local.contributor.affiliationMuller, Holger, University of California
local.contributor.affiliationAndo, Masaki, Kyoto University
local.contributor.authoruidSlagmolen, Bram, u9905035
local.description.notesImported from ARIES
local.identifier.absfor020105 - General Relativity and Gravitational Waves
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationU3488905xPUB699
local.identifier.citationvolume88
local.identifier.doi10.1103/PhysRevD.88.122003
local.identifier.scopusID2-s2.0-84894569241
local.identifier.thomsonID000328692500003
local.type.statusPublished Version

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