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Gravitational-wave astronomy and astrophysics

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dc.contributor.authorKim, C.-
dc.contributor.authorCho, H.S.-
dc.contributor.authorKang, G.-
dc.contributor.authorLee, H.W.-
dc.contributor.authorLee, C.-H.-
dc.contributor.authorLee, H.K.-
dc.date.accessioned2024-02-23T05:30:48Z-
dc.date.available2024-02-23T05:30:48Z-
dc.date.issued2016-
dc.identifier.issn0374-4914-
dc.identifier.issn2289-0041-
dc.identifier.urihttps://scholarworks.bwise.kr/cau/handle/2019.sw.cau/72391-
dc.description.abstractOn September 14, 2015, gravitational waves (GWs) were detected by the LIGO (Laser Interferometer gravitational-wave observatory) detectors in USA. The event (GW150914) is originated from a coalescence of two black holes (BHs) located at 13 billion light years away from the Earth. This is the first direct detection of GWs and the first observation of a BH-BH binary. We overview astrophysical sources that can be detected by km-scale laser interferometers on Earth, summarize astrophysical implications of GW150914, and discuss how to explore a Universe with GWs.-
dc.format.extent11-
dc.language한국어-
dc.language.isoKOR-
dc.publisherKorean Physical Society-
dc.titleGravitational-wave astronomy and astrophysics-
dc.typeArticle-
dc.identifier.doi10.3938/NPSM.66.293-
dc.identifier.bibliographicCitationNew Physics: Sae Mulli, v.66, no.3, pp 293 - 303-
dc.description.isOpenAccessN-
dc.identifier.scopusid2-s2.0-84964662681-
dc.citation.endPage303-
dc.citation.number3-
dc.citation.startPage293-
dc.citation.titleNew Physics: Sae Mulli-
dc.citation.volume66-
dc.type.docTypeArticle-
dc.publisher.location대한민국-
dc.subject.keywordAuthorAstrophysics-
dc.subject.keywordAuthorBayesian inference-
dc.subject.keywordAuthorBlack holes-
dc.subject.keywordAuthorGamma-ray bursts-
dc.subject.keywordAuthorGravitational waves-
dc.subject.keywordAuthorNeutron stars-
dc.subject.keywordAuthorStatistical analysis-
dc.subject.keywordAuthorSupernovae-
dc.description.journalRegisteredClassscopus-
dc.description.journalRegisteredClasskci-
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