Overview of KAGRA: Detector design and construction history
By T.Akutsu, M.Ando, K.Arai, Y.Arai, S.Araki, A.Araya, N.Aritomi, Y.Aso, S.-W.Bae, Y.-B.Bae and 187 more. Progress of Theoretical and Experimental Physics, 2020
699 citations recorded by the source corpus.
KAGRA is a newly built gravitational-wave telescope, a laser interferometer comprising arms with a length of 3 km, located in Kamioka, Gifu, Japan. KAGRA was constructed under the ground and it is operated using cryogenic mirrors that help in reducing the seismic and thermal noise. Both technologies are expected to provide directions for the future of gravitational-wave telescopes. In 2019, KAGRA finished all installations with the designed configuration, which we call the baseline KAGRA. For this occasion, we present an overview of the baseline KAGRA from various viewpoints in a series of articles. In this article, we introduce the design configurations of KAGRA with its historical background.
Subfields: Astronomy and Astrophysics, Geophysics, Ocean Engineering
View Paper: https://www.semanticscholar.org/paper/65a5283eca8cf390a112fd9b899af58aca1f9ff4
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In Astronomy and Astrophysics
- Michela Mapelli
- D. Holz
- Maya Fishbach
- E. Thrane
- N. Giacobbo
- Ilya Mandel
- R. O’Shaughnessy
- Luca Baiotti
In Geophysics
- E. Thrane
- Luca Baiotti
- S. Nissanke
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In Ocean Engineering
- E. Thrane
- Rana X. Adhikari
- D. Holz
- Maya Fishbach
- P. Jaranowski
- R. O’Shaughnessy
- Stephen Fairhurst
- Walter Del Pozzo
Citations in the corpus
- GW231123: A Binary Black Hole Merger with Total Mass 190–265 M⊙ (2025, positive): “From 2015 to 2020 the LIGO-Virgo-KAGRA Collab-oration identified 69 gravitational-wave signals from binary black hole mergers with false alarm rates below one per year (Aasi et al. 2015; Acernese et al. 2015; Abbott et al. 2020d; Akutsu et al. 2020; Abbott et al. 2023a).”