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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3830
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dc.contributor.authorAndo, Masaki-
dc.contributor.authorKawamura, Seiji-
dc.contributor.authorSato, Shuichi-
dc.contributor.authorNakamura, Takashi-
dc.contributor.authorFujita, Ryuichi-
dc.contributor.author+40 Co-authors-
dc.date.accessioned2009-08-01T11:39:34Z-
dc.date.available2009-08-01T11:39:34Z-
dc.date.issued2009-05-
dc.identifier.citationClassical and Quantum Gravity, 2009, Vol. 26, p094019en
dc.identifier.issn0264-9381-
dc.identifier.issn1361-6382 (online)-
dc.identifier.urihttp://hdl.handle.net/2289/3830-
dc.descriptionRestricted Accessen
dc.description.abstractDECIGO pathfinder (DPF) is a milestone satellite mission for DECIGO (DECi-hertz Interferometer Gravitational wave Observatory), which is a future space gravitational wave antenna. DECIGO is expected to provide fruitful insights into the universe, particularly about dark energy, the formation mechanism of supermassive black holes and the inflation of the universe. Since DECIGO will be an extremely challenging mission, which will be formed by three drag-free spacecraft with 1000 km separation, it is important to increase the technical feasibility of DECIGO before its planned launch in 2024. Thus, we are planning to launch two milestone missions: DPF and pre-DECIGO. In this paper, we review the conceptual design and current status of the first milestone mission, DPF.en
dc.language.isoenen
dc.publisherIOP Publishing Ltd.en
dc.relation.urihttp://dx.doi.org/10.1088/0264-9381/26/9/094019en
dc.relation.urihttp://adsabs.harvard.edu/abs/2009CQGra..26i4019Aen
dc.rights2009 IOP Publishingen
dc.subjectGravitational wave detectors and experimentsen
dc.subjectSupergiant starsen
dc.subjectInterferometryen
dc.subjectDark energyen
dc.subjectGravitational radiation detectors; mass spectrometers; and other instrumentation and techniquesen
dc.subjectBlack holesen
dc.titleDECIGO pathfinderen
dc.typeArticleen
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