Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/53980
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dc.contributor.authorBlair, D.en
dc.contributor.authorBarriga, P.en
dc.contributor.authorBrooks, A.en
dc.contributor.authorCharlton, P.en
dc.contributor.authorCoward, D.en
dc.contributor.authorDumas, J.en
dc.contributor.authorFan, Y.en
dc.contributor.authorGalloway, D.en
dc.contributor.authorGras, S.en
dc.contributor.authorHosken, D.en
dc.contributor.authorHowell, E.en
dc.contributor.authorHughes, S.en
dc.contributor.authorJu, L.en
dc.contributor.authorMcClelland, D.en
dc.contributor.authorMelatos, A.en
dc.contributor.authorMiao, H.en
dc.contributor.authorMunch, J.en
dc.contributor.authorScott, S.en
dc.contributor.authorSlagmolen, B.en
dc.contributor.authorVeitch, P.en
dc.contributor.authorWen, L.en
dc.contributor.authorWebb, J.en
dc.contributor.authorWooley, A.en
dc.contributor.authorVan, Z.en
dc.contributor.authorZhao, C.en
dc.date.issued2008en
dc.identifier.citationProceedings of the 7th Edoardo Amaldi Conference on Gravitational Waves (Amaldi7); Journal of Physics: Conference Series, vol. 122, 2008 / vol.122, pp.1-6en
dc.identifier.issn1742-6588en
dc.identifier.issn1742-6596en
dc.identifier.urihttp://hdl.handle.net/2440/53980-
dc.description.abstractThe proposed southern hemisphere gravitational wave detector AIGO increases the projected average baseline of the global array of ground based gravitational wave detectors by a factor ~4. This allows the world array to be substantially improved. The orientation of AIGO allows much better resolution of both wave polarisations. This enables better distance estimates for inspiral events, allowing unambiguous optical identification of host galaxies for about 25% of neutron star binary inspiral events. This can allow Hubble Law estimation without optical identification of an outburst, and can also allow deep exposure imaging with electromagnetic telescopes to search for weak afterglows. This allows independent estimates of cosmological acceleration and dark energy as well as improved understanding of the physics of neutron star and black hole coalescences. This paper reviews and summarises the science benefits of AIGO and presents a preliminary conceptual design.en
dc.description.statementofresponsibilityD G Blair, P Barriga, A F Brooks, P Charlton, D Coward, J-C Dumas, Y Fan, D Galloway, S Gras, D J Hosken, E Howell, S Hughes, L Ju, D E McClelland, A Melatos, H Miao, J Munch, S M Scott, B J J Slagmolen, P J Veitch, L Wen, J K Webb, A Wolley, Z Yan and C Zhaoen
dc.language.isoenen
dc.publisherInstitute of Physics Publishingen
dc.titleThe science benefits and preliminary design of the Southern hemisphere gravitational wave detector AIGOen
dc.typeConference paperen
dc.identifier.rmid0020084209en
dc.contributor.conferenceEdoardo Amaldi Conference on Gravitational Waves (Amaldi) (08 Jul 2007 : Sydney NSW)en
dc.identifier.doi10.1088/1742-6596/122/1/012001en
dc.publisher.placeUKen
dc.identifier.pubid40874-
pubs.library.collectionPhysics publicationsen
pubs.verification-statusVerifieden
pubs.publication-statusPublisheden
dc.identifier.orcidVeitch, P. [0000-0002-2597-435X]en
Appears in Collections:Physics publications
Environment Institute publications

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