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- dc.contributor.author
- LIGO Scientific Collaboration
- dc.contributor.author
- 강궁원
- dc.contributor.author
- 김정리
- dc.contributor.author
- 김지웅
- dc.contributor.author
- 장행진
- dc.contributor.author
- 조희석
- dc.date.accessioned
- 2019-08-28T07:42:09Z
- dc.date.available
- 2019-08-28T07:42:09Z
- dc.date.issued
- 2017-02-23
- dc.identifier.issn
- 0264-9381
- dc.identifier.uri
- https://repository.kisti.re.kr/handle/10580/14681
- dc.identifier.uri
- http://www.ndsl.kr/ndsl/search/detail/article/articleSearchResultDetail.do?cn=NART78516490
- dc.description.abstract
- The second-generation of gravitational-wave detectors are just startingoperation, and have already yielding their first detections. Research is nowconcentrated on how to maximize the scientific potential of gravitationalwaveastronomy. To support this effort, we present here design targets fora new generation of detectors, which will be capable of observing compactbinary sources with high signal-to-noise ratio throughout the Universe.
- dc.language
- eng
- dc.relation.ispartofseries
- Classical and Quantum Gravity
- dc.title
- Exploring the sensitivity of next generation gravitational wave detectors
- dc.citation.number
- 4
- dc.citation.startPage
- 044001
- dc.citation.volume
- 34
- dc.subject.keyword
- gravitational waves
- dc.subject.keyword
- cosmic explorer
- dc.subject.keyword
- LIGO
- Appears in Collections:
- 7. KISTI 연구성과 > 학술지 발표논문
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