Showing papers by "F. Kawazoe published in 2019"
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Nagoya University1, Kyoto University2, University of Tokyo3, National Institutes of Natural Sciences, Japan4, Osaka City University5, Japan Aerospace Exploration Agency6, University of Electro-Communications7, Hosei University8, University of Birmingham9, Waseda University10, California Institute of Technology11, Hirosaki University12, Nihon University13, Fukuoka University14, Ochanomizu University15, Tokyo Keizai University16, University of Lisbon17, Kyoto Sangyo University18, Rikkyo University19, Osaka University20, Yokohama National University21, Tokai University22, National Institute of Information and Communications Technology23, National Institute of Advanced Industrial Science and Technology24, Kindai University25, National Science Foundation26, Leibniz University of Hanover27, Setsunan University28, Liverpool John Moores University29, Hiroshima University30, Louisiana State University31, Akita Prefectural University32, Ryukoku University33, National Defense Academy of Japan34, Niigata University35, Graduate University for Advanced Studies36, Kyushu University37, Osaka Institute of Technology38, Tokyo Institute of Technology39, Tohoku University40, Kumamoto University41, Nagaoka University of Technology42, University of the Ryukyus43, Tokyo University of Science44, Montana State University45
TL;DR: The B-DECIGO as discussed by the authors is a small-scale version of DECIGO with a sensitivity slightly worse than that of DECI-HERT, yet good enough to provide frequent detection of gravitational waves.
Abstract: DECi-hertz Interferometer Gravitational-wave Observatory (DECIGO) is a future Japanese space gravitational-wave antenna. The most important objective of DECIGO, among various sciences to be aimed at, is to detect gravitational waves coming from the inflation of the universe. DECIGO consists of four clusters of spacecraft, and each cluster consists of three spacecraft with three Fabry–Perot Michelson interferometers. As a pathfinder mission of DECIGO, B-DECIGO will be launched, hopefully in the 2020s, to demonstrate technologies necessary for DECIGO as well as to lead to fruitful multimessenger astronomy. B-DECIGO is a small-scale or simpler version of DECIGO with the sensitivity slightly worse than that of DECIGO, yet good enough to provide frequent detection of gravitational waves.
75 citations