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13 results on '"Miyakawa, Osamu"'

1. Design and experimental demonstration of a laser modulation system for future gravitational-wave detectors

Author

Yamamoto, Kohei, Ge, Gui-Guo, Fujikawa, Yuta, Fujii, Nobuyuki, Kokeyama, Keiko, Michimura, Yuta, Enomoto, Yutaro, Nakano, Masayuki, Uehara, Tomoyuki, Somiya, Kentaro, Izumi, Kiwamu, Miyakawa, Osamu, Yamamoto, Takahiro, Yokozawa, Takaaki, and Kajita, Takaaki

Subjects
Physics - Instrumentation and Detectors, Physics and Astronomy (miscellaneous), FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Mach–Zehnder interferometer, 01 natural sciences, Noise (electronics), General Relativity and Quantum Cosmology, Optics, 0103 physical sciences, Astronomical interferometer, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, laser interferometer, 010308 nuclear & particles physics, business.industry, Quantum limit, Quantum noise, Detector, Instrumentation and Detectors (physics.ins-det), detuning, Interferometry, modulation, gravitational waves, Modulation, business, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

著者人数: 15名, Accepted: 2019-09-13, 資料番号: SA1190121000

Published
2019

4. The Japanese space gravitational wave antenna - DECIGO

Author

Kawamura, Seiji, Ando, Masaki, Nakamura, Takashi, Tsubono, Kimio, Tanaka, Takahiro, Funaki, Iklkoh, Seto, Naoki, Numata, Kenji, Sato, Shuichi, Ioka, Kunihito, Kanda, Nobuyuki, Takashima, Takeshi, Agatsuma, Kazuhiro, Akutsu, Tomotada, Akutsu, Tomomi, Aoyanagi, Koh-suke, Arai, Koji, Arase, Yuta, Araya, Akito, Asada, Hideki, Aso, Yoichi, Chiba, Takeshi, Ebisuzaki, Toshikazu, Fukushima, Mitsuhiro, Futamase, Toshifumi, Ganzu, Katsuhiko, Harada, Tomohiro, Hashimoto, Tatsuaki, Hayama, Kazuhiro, Hikida, Wataru, Himemoto, Yoshiaki, Hirabayashi, Hisashi, Hiramatsu, Takashi, Hong, Feng-Lei, Horisawa, Hideyuki, Hosokawa, Mizuhiko, Ichiki, Kiyotomo, Ikegami, Takeshi, Inoue, Kaiki T., Ishidoshiro, Koji, Ishihara, Hideki, Ishikawa, Takehiko, Ishizaki, Hideharu, Ito, Hiroyuki, Itoh, Yousuke, Kamagasako, Shogo, Kawashima, Nobuki, Kawazoe, Fumiko, Kirihara, Hiroyuki, Kishimoto, Naoko, Kiuchi, Kenta, Kobayashi, Shiho, Kohri, Kazunori, Koizumi, Hiroyuki, Kojima, Yasufumi, Kokeyama, Keiko, Kokuyama, Wataru, Kotake, Kei, Kozai, Yoshihide, Kudoh, Hideaki, Kunimori, Hiroo, Kuninaka, Hitoshi, Kuroda, Kazuaki, Maeda, Kei-ichi, Matsuhara, Hideo, Mino, Yasushi, Miyakawa, Osamu, Miyoki, Shinji, Morimoto, Mutsuko Y., Morioka, Tomoko, Morisawa, Toshiyuki, Moriwaki, Shigenori, Mukohyama, Shinji, Musha, Mitsuru, Nagano, Shigeo, Naito, Isao, Nakagawa, Noriyasu, Nakamura, Kouji, Nakano, Hiroyuki, Nakao, Kenichi, Nakasuka, Shinichi, Nakayama, Yoshinori, Nishida, Erina, Nishiyama, Kazutaka, Nishizawa, Atsushi, Niwa, Yoshito, Ohashi, Masatake, Ohishi, Naoko, Ohkawa, Masashi, Okutomi, Akira, Onozato, Kouji, Oohara, Kenichi, Sago, Norichika, Saijo, Motoyuki, Sakagami, Masaaki, Sakai, Shin-ichiro, Sakata, Shihori, Sasaki, Misao, Sato, Takashi, Shibata, Masaru, Shinkai, Hisaaki, Somiya, Kentaro, Sotani, Hajime, Sugiyama, Naoshi, Suwa, Yudai, Tagoshi, Hideyuki, Takahashi, Kakeru, Takahashi, Keitaro, Takahashi, Tadayuki, Tahahashi, Hirotaka, Takahashi, Ryuichi, Takahashi, Ryutaro, Takamori, Akiteru, Takano, Tadashi, Taniguchi, Keisuke, Taruya, Atsushi, Tashiro, Hiroyuki, Tokuda, Mitsuru, Tokunari, Masao, Toyoshima, Morio, Tsujikawa, Shinji, Tsunesada, Yoshiki, Ueda, Ken-ichi, Utashima, Masayoshi, Yamakawa, Hiroshi, Yamamoto, Kazuhiro, Yamazaki, Toshitaka, Yokoyama, Jun'ichi, Yoo, Chul-Moon, Yoshida, Shijun, and Yoshino, Taizoh

Subjects
Physics::General Physics, Astrophysics::Instrumentation and Methods for Astrophysics
Abstract

DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. The goal of DECIGO is to detect gravitational waves from various kinds of sources mainly between 0.1 Hz and 10 Hz and thus to open a new window of observation for gravitational wave astronomy. DECIGO will consist of three drag-free spacecraft, 1000 km apart from each other, whose relative displacements are measured by a Fabry—Perot Michelson interferometer. We plan to launch DECIGO pathfinder first to demonstrate the technologies required to realize DECIGO and, if possible, to detect gravitational waves from our galaxy or nearby galaxies.

Published
2008

5. Abranding increases oxygen and hardness of titanium surface

Author

Miyakawa, Osamu, Okawa, Seigo, and Kobayashi, Masayoshi

Subjects
Titanium, Oxygen, Abrading
Abstract

CP Ti was mirror-polished and then abraded with waterproof SiC papers of two different grit sizes: 16 and 3μm. Aspolished and abraded surfaces were characterized by means of EPMA, XPS, XRD, and hardness test. Oxygen in the mirror-polished surface was uniformly distributed at the lowest level. Comparatively, abrading with SiC papers increased the surface oxygen amount and hardness. Owing to its excellent abrasivity, the coarse grit efficiently scratched the surface and hindered the regenerated oxide film from growing thick, but allowed only the metal-oxide interfacial gradient zone to extend. But, the fine grit merely rubbed the surface and allowed both the oxide film and interfacial zone to extend. Further, the surface appeared to be lightly yellow-colored, suggesting that the oxide film was thicker, probably within 10nm, than the nominal one. When compared with the bulk, the interfacial zone was rich in oxygen and therefore subjected to high coherency strain, which was introduced to relieve the great lattice mismatch between the outer and inner layers of titanium substrate. Effects of solute oxygen hardening and strain hardening were speculated to be responsible for the surface hardening of both SiC-abraded surfaces. In conclusion, abrading with a coarse grit led to accumulation of a high, non-uniform strain in the titanium substrate, thereby hardening the surface further.

Published
2006

7. Thermal-noise-limited underground interferometer CLIO

Author

Agatsuma, Kazuhiro, Arai, Koji, Fujimoto, Masa-Katsu, Kawamura, Seiji, Kuroda, Kazuaki, Miyakawa, Osamu, Miyoki, Shinji, Ohashi, Masatake, Suzuki, Toshikazu, Takahashi, Ryutaro, Tatsumi, Daisuke, Telada, Souichi, Uchiyama, Takashi, Yamamoto, Kazuhiro, and collaborators, CLIO

Subjects
Physics, Physics and Astronomy (miscellaneous), business.industry, Physics::Instrumentation and Detectors, Pendulum, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Laser, Noise (electronics), General Relativity and Quantum Cosmology, law.invention, Telescope, Interferometry, Optics, Observatory, law, Magnet, Interferometric gravitational wave detector, business
Abstract

We report on the current status of CLIO (Cryogenic Laser Interferometer Observatory), which is a prototype interferometer for LCGT (Large Scale Cryogenic Gravitational-Wave Telescope). LCGT is a Japanese next-generation interferometric gravitational wave detector featuring the use of cryogenic mirrors and a quiet underground site. The main purpose of CLIO is to demonstrate a reduction of the mirror thermal noise by cooling the sapphire mirrors. CLIO is located in an underground site of the Kamioka mine, 1000 m deep from the mountain top, to verify its advantages. After a few years of commissioning work, we have achieved a thermal-noise-limited sensitivity at room temperature. One of the main results of noise hunting was the elimination of thermal noise caused by a conductive coil-holder coupled with a pendulum through magnets., Comment: 10 pages, 6 figures, Proceedings of the 8th Edoardo Amaldi Conference on Gravitational Waves

Published
2009
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8. DECIGO pathfinder

Author

Ando, Masaki, Kawamura, Seiji, Nakamura, Takashi, Tsubono, Kimio, Tanaka, Takahiro, Funaki, Ikkoh, Seto, Naoki, Numata, Kenji, Sato, Shuichi, Ioka, Kunihito, Kanda, Nobuyuki, Takashima, Takeshi, Agatsuma, Kazuhiro, Akutsu, Tomotada, Akutsu, Tomomi, Aoyanagi, Koh-suke, Arai, Koji, Arase, Yuta, Araya, Akito, Asada, Hideki, Aso, Yoichi, Chiba, Takeshi, Ebisuzaki, Toshikazu, Enoki, Motohiro, Eriguchi, Yoshiharu, Fujimoto, Masa-Katsu, Fujita, Ryuichi, Fukushima, Mitsuhiro, Futamase, Toshifumi, Ganzu, Katsuhiko, Harada, Tomohiro, Hashimoto, Tatsuaki, Hayama, Kazuhiro, Hikida, Wataru, Himemoto, Yoshiaki, Hirabayashi, Hisashi, Hiramatsu, Takashi, Hong, Feng-Lei, Horisawa, Hideyuki, Hosokawa, Mizuhiko, Ichiki, Kiyotomo, Ikegami, Takashi, Inoue, Kaiki T., Ishidoshiro, Koji, Ishihara, Hideki, Ishikawa, Takehiko, Ishizaki, Hideharu, Ito, Hiroyuki, Itoh, Yousuke, Kamagasako, Shogo, Kawashima, Nobuki, Kawazoe, Fumiko, Kirihara, Hiroyuki, Kishimoto, Naoko, Kiuchi, Kenta, Kobayashi, Shiho, Kohri, Kazunori, Koizumi, Hiroyuki, Kojima, Yasufumi, Kokeyama, Keiko, Kokuyama, Wataru, Kotake, Kei, Kozai, Yoshihide, Kudoh, Hideaki, Kunimori, Hiroo, Kuninaka, Hitoshi, Kuroda, Kazuaki, Maeda, Kei-ichi, Matsuhara, Hideo, Mino, Yasushi, Miyakawa, Osamu, Miyoki, Shinji, Morimoto, Mutsuko Y., Morioka, Tomoko, Morisawa, Toshiyuki, Moriwaki, Shigenori, Mukohyama, Shinji, Musha, Mitsuru, Nagano, Shigeo, Naito, Isao, Nakagawa, Noriyasu, Nakamura, Kouji, Nakano, Hiroyuki, Nakao, Kenichi, Nakasuka, Shinichi, Nakayama, Yoshinori, Nishida, Erina, Nishiyama, Kazutaka, Nishizawa, Atsushi, Niwa, Yoshito, Ohashi, Masatake, Ohishi, Naoko, Ohkawa, Masashi, Okutomi, Akira, Onozato, Kouji, Oohara, Kenichi, Sago, Norichika, Saijo, Motoyuki, Sakagami, Masaaki, Sakai, Shin-ichiro, Sakata, Shihori, Sasaki, Misao, Sato, Takashi, Shibata, Masaru, Shinkai, Hisaaki, Somiya, Kentaro, Sotani, Hajime, Sugiyama, Naoshi, Suwa, Yudai, Tagoshi, Hideyuki, Takahashi, Kakeru, Takahashi, Keitaro, Takahashi, Tadayuki, Takahashi, Hirotaka, Takahashi, Ryuichi, Takahashi, Ryutaro, Takamori, Akiteru, Takano, Tadashi, Taniguchi, Keisuke, Taruya, Atsushi, Tashiro, Hiroyuki, Tokuda, Mitsuru, Tokunari, Masao, Toyoshima, Morio, Tsujikawa, Shinji, Tsunesada, Yoshiki, Ueda, Ken-ichi, Utashima, Masayoshi, Yamakawa, Hiroshi, Yamamoto, Kazuhiro, Yamazaki, Toshitaka, Yokoyama, Jun'ichi, Yoo, Chul-Moon, Yoshida, Shijun, and Yoshino, Taizoh

Subjects
History, Computer Science Applications, Education
Abstract

DECIGO 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 us fruitful insights into the universe, in particular about dark energy, a formation mechanism of supermassive black holes, and the inflation of the universe. Since DECIGO will be an extremely large mission which will formed by three drag-free spacecraft with 1000m separation, it is significant to gain the technical feasibility of DECIGO before its planned launch in 2024. Thus, we are planning to launch two milestone missions: DPF and pre-DECIGO. The conceptual design and current status of the first milestone mission, DPF, are reviewed in this article.

Published
2008

9. 小型重力波観測衛星 DPF

Author

Kishimoto, Naoko, Kudoh, Hideaki, Kuninaka, Hitoshi, Kunimori, Hiroo, Kuroda, Kazuaki, Koizumi, Hiroyuki, Kohri, Kazunori, Kokuyama, Wataru, Kokeyama, Keiko, Kozai, Yoshihide, Sakai, Shinichiro, Sakagami, Masaaki, Sakata, Shihori, Sasaki, Tadashi, Shibata, Masaru, Shinkai, Hisaaki, Sugiyama, Naoshi, Suwa, Yudai, Somiya, Kentaro, Sotani, Hajime, Takano, Tadashi, Takahashi, Kakeru, Takahashi, Keitaro, Takahashi, Tadayuki, Takahashi, Hirotaka, Takahashi, Ryuich, Takahashi, Ryutaro, Takamori, Akiteru, Tagoshi, Hideyuki, Taniguchi, Keisuke, Taruya, Atsushi, Chiba, Takeshi, Tsujikawa, Shinji, Tsunesada, Yoshiki, Tokunari, Masao, Toyoshima, Morio, Nakao, Ken-ichi, Nakasuka, Shinichi, Nakano, Hiroyuki, Nagano, Shigeo, Nakayama, Yoshinori, Nishiyama, Kazutaka, Niwa, Yoshito, Hashimoto, Tatsuaki, Harada, Tomohiro, Hikida, Wataru, Himemoto, Yoshiaki, Hirabayashi, Hisashi, Hiramatsu, Takashi, Fukushima, Mitsuhiro, Fujita, Ryuichi, Fujimoto, Masa-Katsu, Futamase, Toshifumi, Hosokawa, Mizuhiko, Horisawa, Hideyuki, Maeda, Keiichi, Matsuhara, Hideo, Miyakawa, Osamu, Miyoki, Shinji, Musha, Mitsuru, Morimoto, Mutsuko Y., Moriwaki, Shigenori, Yamakawa, Hiroshi, Yamazaki, Toshitaka, Yamamoto, Kazuhiro, Yokoyama, Jun'ichi, Yoshino, Taizo, Ando, Masaki, Kawamura, Seiji, Nakamura, Takashi, Tsubono, Kimio, Tanaka, Takahiro, Funaki, Ikkoh, Seto, Naoki, Numata, Kenji, Sato, Syuichi, Kanda, Nobuyuki, Ioka, Kunihito, Takashima, Takeshi, Aoyanagi, Koh-suke, Agatsuma, Kazuhiro, Akutsu, Tomotada, Asada, Hideki, Aso, Yoichi, Arai, Koji, Araya, Akito, Ikegami, Takeshi, Ishikawa, Takehiko, Ishizaki, Hideharu, Ishidoshiro, Koji, Ishihara, Mitsunori, Ichiki, Kiyotomo, Ito, Hiroyuki, Ito, Yosuke, Ueda, Kenichi, Utashima, Masayoshi, Enoki, Motohiro, Ebisuzaki, Tosikazu, Eriguchi, Yoshiharu, Ohishi, Naoko, Ohkawa, Masashi, Ohashi, Masatake, Oohara, Kenichi, Okutomi, Akira, Kawashima, Nobuki, and Kawazoe, Fumiko

Abstract

第8回宇宙科学シンポジウム (2008年1月8日-9日. 宇宙航空研究開発機構宇宙科学研究本部(JAXA)(ISAS)相模原キャンパス), 相模原市, 神奈川県, 8ｔh Space Science Symposium (January 8-9, 2008. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS)Sagamihara Campus), Sagamihara, Kanagawa Japan, 著者人数: 135名, 資料番号: SA6000056016, レポート番号: S2-10

Published
2008

10. スペース重力波アンテナDECIGO

Author

Kishimoto, Naoko, Kudoh, Hideaki, Kuninaka, Hitoshi, Kunimori, Hiroo, Kuroda, Kazuaki, Koizumi, Hiroyuki, Kohri, Kazunori, Kokuyama, Wataru, Kokeyama, Keiko, Kozai, Yoshihide, Sakai, Shinichiro, Sakagami, Masaaki, Sakata, Shihori, Sasaki, Tadashi, Shibata, Masaru, Shinkai, Hisaaki, Sugiyama, Naoshi, Suwa, Yudai, Somiya, Kentaro, Sotani, Hajime, Takano, Tadashi, Takahashi, Kakeru, Takahashi, Keitaro, Takahashi, Tadayuki, Takahashi, Hirotaka, Takahashi, Ryuich, Takahashi, Ryutaro, Takamori, Akiteru, Tagoshi, Hideyuki, Taniguchi, Keisuke, Taruya, Atsushi, Chiba, Takeshi, Tsujikawa, Shinji, Tsunesada, Yoshiki, Tokunari, Masao, Toyoshima, Morio, Nakao, Ken-ichi, Nakasuka, Shinichi, Nakano, Hiroyuki, Nagano, Shigeo, Nakayama, Yoshinori, Nishiyama, Kazutaka, Niwa, Yoshito, Hashimoto, Tatsuaki, Harada, Tomohiro, Hikida, Wataru, Himemoto, Yoshiaki, Hirabayashi, Hisashi, Hiramatsu, Takashi, Fukushima, Mitsuhiro, Fujita, Ryuichi, Fujimoto, Masa-Katsu, Futamase, Toshifumi, Hosokawa, Mizuhiko, Horisawa, Hideyuki, Maeda, Keiichi, Matsuhara, Hideo, Miyakawa, Osamu, Miyoki, Shinji, Musha, Mitsuru, Morimoto, Mutsuko Y., Moriwaki, Shigenori, Yamakawa, Hiroshi, Yamazaki, Toshitaka, Yamamoto, Kazuhiro, Yokoyama, Jun'ichi, Yoshino, Taizo, Kawamura, Seiji, Ando, Masaki, Nakamura, Takashi, Tsubono, Kimio, Tanaka, Takahiro, Funaki, Ikkoh, Seto, Naoki, Numata, Kenji, Sato, Syuichi, Kanda, Nobuyuki, Ioka, Kunihito, Takashima, Takeshi, Aoyanagi, Koh-suke, Agatsuma, Kazuhiro, Akutsu, Tomotada, Asada, Hideki, Aso, Yoichi, Arai, Koji, Araya, Akito, Ikegami, Takeshi, Ishikawa, Takehiko, Ishizaki, Hideharu, Ishidoshiro, Koji, Ishihara, Mitsunori, Ichiki, Kiyotomo, Ito, Hiroyuki, Ito, Yosuke, Ueda, Kenichi, Utashima, Masayoshi, Enoki, Motohiro, Ebisuzaki, Tosikazu, Eriguchi, Yoshiharu, Ohishi, Naoko, Ohkawa, Masashi, Ohashi, Masatake, Oohara, Kenichi, Okutomi, Akira, Kawashima, Nobuki, and Kawazoe, Fumiko

Abstract

第8回宇宙科学シンポジウム (2008年1月8日-9日. 宇宙航空研究開発機構宇宙科学研究本部(JAXA)(ISAS)相模原キャンパス), 相模原市, 神奈川県, 8ｔh Space Science Symposium (January 8-9, 2008. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS)Sagamihara Campus), Sagamihara, Kanagawa Japan, 著者人数: 135名, 資料番号: SA6000056110, レポート番号: P2-78

Published
2008

11. Measurement of Optical Response of a Detuned Resonant Sideband Extraction Interferometer

Author

Miyakawa, Osamu, Ward, Robert, Adhikari, Rana, Evans, Matthew, Abbott, Benjamin, Bork, Rolf, Busby, Daniel, Heefner, Jay, Ivanov, Alexander, Smith, Michael, Taylor, Robert, Vass, Stephen, Weinstein, Alan, Varvella, Monica, Kawamura, Seiji, Kawazoe, Fumiko, Sakata, Shihori, and Mow-Lowry, Conor

Subjects
FOS: Physical sciences, Physics::Optics, General Relativity and Quantum Cosmology (gr-qc), General Relativity and Quantum Cosmology
Abstract

We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) interferometer with power recycling. The purpose of the detuned RSE configuration is to manipulate and optimize the optical response of the interferometer to differential displacements (induced by gravitational waves) as a function of frequency, independently of other parameters of the interferometer. The design of our interferometer results in an optical gain with two peaks: an RSE optical resonance at around 4 kHz and a radiation pressure induced optical spring at around 41 Hz. We have developed a reliable procedure for acquiring lock and establishing the desired optical configuration. In this configuration, we have measured the optical response to differential displacement and found good agreement with predictions at both resonances and all other relevant frequencies. These results build confidence in both the theory and practical implementation of the more complex optical configuration being planned for Advanced LIGO., 6 pages, 4 figures, for submission to Phys Rev Letters

Published
2006

12. Observation results by the TAMA300 detector on gravitational wave bursts from stellar-core collapses

Author

Beyersdorf, Peter, Iida, Yukiyoshi, Zhu, Zong-Hong, Barton, Mark A., Heinzel, Gerhard, Iguchi, Hideo, Karasawa, Yoshikazu, Kawamura, Mari, Kojima, Yasufumi, Matsuda, Namio, Miura, Kazuyuki, Nagayama, Yoshitaka, Sato, Kouichi, Soida, Kenji, Taylor, C. T., Waseda, Koichi, Yoshida, Tatsuru, Ando, Masaki, Arai, Koji, Aso, Youichi, Hayama, Kazuhiro, Kanda, Nobuyuki, Kawamura, Seiji, Kondo, Kazuhiro, Mio, Norikatsu, Miyoki, Shinji, Moriwaki, Shigenori, Nagano, Shigeo, Numata, Kenji, Sato, Shuichi, Somiya, Kentaro, Tagoshi, Hideyuki, Takahashi, Hirotaka, Takahashi, Ryutaro, Tatsumi, Daisuke, Tsunesada, Yoshiki, Akutsu, Tomomi, Akutsu, Tomotada, Araya, Akito, Asada, Hideki, Fujiki, Youhei, Fujimoto, Masa-Katsu, Fujita, Ryuichi, Fukushima, Mitsuhiro, Futamase, Toshifumi, Hamuro, Yusaku, Haruyama, Tomiyoshi, Hayakawa, Hideaki, Horikoshi, Gen'ichi, Ioka, Kunihito, Ishitsuka, Hideki, Kamikubota, Norihiko, Kaneyama, Takaharu, Kasahara, Kunihiko, Kasai, Taketoshi, Katsuki, Mayu, Kawabe, Keita, Kawashima, Nobuki, Kawazoe, Fumiko, Kokeyama, Keiko, Kozai, Yoshihide, Kudoh, Hideaki, Kuroda, Kazuaki, Kuwabara, Takashi, Miyakawa, Osamu, Miyama, Shoken, Mizusawa, Hiromi, Musha, Mitsuru, Nakagawa, Ken'ichi, Nakamura, Takashi, Nakano, Hiroyuki, Nakao, Ken-ichi, Nishi, Yuhiko, Ogawa, Yujiro, Ohashi, Masatake, Ohishi, Naoko, Okutomi, Akira, Oohara, Ken-ichi, Otsuka, Shigemi, Saito, Yoshio, Sakata, Shihori, Sasaki, Misao, Sato, Nobuaki, Sato, Youhei, Seki, Hidetsugu, Sekido, Aya, Seto, Naoki, Shibata, Masaru, Shinkai, Hisaaki, Shintomi, Takakazu, Suzuki, Toshikazu, Takamori, Akiteru, Takemoto, Shuzo, Takeno, Kohei, Tanaka, Takahiro, Taniguchi, Keisuke, Taniguchi, Shinsuke, Tanji, Toru, Telada, Souichi, Tochikubo, Kuniharu, Tokunari, Masao, Tomaru, Takayuki, Tsubono, Kimio, Tsuda, Nobuhiro, Uchiyama, Takashi, Ueda, Akitoshi, Ueda, Ken-ichi, Usui, Fumihiko, Watanabe, Yuko, Yakura, Hiromi, Yamamoto, Akira, Yamamoto, Kazuhiro, Yamazaki, Toshitaka, Yanagi, Yuriko, Yoda, Tatsuo, and Yokoyama, Jun'ichi

Subjects
Physics, Nuclear and High Energy Physics, Gravitational-wave observatory, Gravitational wave, Detector, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, General Relativity and Quantum Cosmology, Particle detector, Cosmology, Chirp, Waveform, Interferometric gravitational wave detector
Abstract

著者人数: 116名, 資料番号: SA1004012000

Published
2005

13. The Japanese space gravitational wave antenna: DECIGO

Author

Chen, Dan, Hong, Feng-Lei, Ichiki, Kiyotomo, Ikegami, Takeshi, Inoue, Kaiki T., Ishidoshiro, Koji, Ishihara, Hideki, Ishizaki, Hideharu, Ito, Hiroyuki, Itoh, Yousuke, Izumi, Kiwamu, Kawashima, Nobuki, Kawazoe, Fumiko, Kishimoto, Naoko, Kiuchi, Kenta, Kobayashi, Shiho, Kohri, Kazunori, Kojima, Yasufumi, Kokeyama, Keiko, Kokuyama, Wataru, Kotake, Kei, Kozai, Yoshihide, Kunimori, Hiroo, Kuroda, Kazuaki, Kuroyanagi, Sachiko, Maeda, Kei-ichi, Matsumoto, Nobuyuki, Michimura, Yuta, Miyakawa, Osamu, Miyamoto, Umpei, Miyoki, Shinji, Morisawa, Toshiyuki, Moriwaki, Shigenori, Mukohyama, Shinji, Musha, Mitsuru, Nagano, Shigeo, Naito, Isao, Nakamura, Kouji, Nakano, Hiroyuki, Nakao, Kenichi, Nakasuka, Shinichi, Nakayama, Yoshinori, Nakazawa, Kazuhiro, Nishida, Erina, Nishizawa, Atsushi, Niwa, Yoshito, Noumi, Taiga, Obuchi, Yoshiyuki, Ohashi, Masatake, Ohishi, Naoko, Ohkawa, Masashi, Okada, Kenshi, Okada, Norio, Oohara, Kenichi, Sago, Norichika, Saijo, Motoyuki, Saito, Ryo, Sakagami, Masaaki, Sakata, Shihori, Sasaki, Misao, Sato, Takashi, Shibata, Masaru, Shinkai, Hisaaki, Shoda, Ayaka, Somiya, Kentaro, Sotani, Hajime, Sugiyama, Naoshi, Suwa, Yudai, Suzuki, Rieko, Tagoshi, Hideyuki, Takahashi, Fuminobu, Takahashi, Kakeru, Takahashi, Keitaro, Takahashi, Ryutaro, Takahashi, Ryuichi, Takahashi, Hirotaka, Akiteru, Takamori, Takano, Tadashi, Tanaka, Nobuyuki, Taniguchi, Keisuke, Taruya, Atsushi, Tashiro, Hiroyuki, Torii, Yasuo, Toyoshima, Morio, Tsujikawa, Shinji, Tsunesada, Yoshiki, Ueda, Akitoshi, Ueda, Ken-ichi, Wakabayashi, Yaka, Yagi, Kent, Yamakawa, Hiroshi, Yamamoto, Kazuhiro, Yamazaki, Toshitaka, Yoo, Chul-Moon, Yoshida, Shijun, Yoshino, Taizoh, Sun, Ke-Xun, Kawamura, Seiji, Ando, Masaki, Seto, Naoki, Sato, Shuichi, Nakamura, Takashi, Tsubono, Kimio, Kanda, Nobuyuki, Tanaka, Takahiro, Yokoyama, Jun'ichi, Funaki, Ikkoh, Numata, Kenji, Ioka, Kunihito, Takashima, Takeshi, Agatsuma, Kazuhiro, Akutsu, Tomotada, Aoyanagi, Koh-suke, Arai, Koji, Araya, Akito, Asada, Hideki, Aso, Yoichi, Chiba, Takeshi, Ebisuzaki, Toshikazu, Ejiri, Yumiko, Enoki, Motohiro, Eriguchi, Yoshiharu, Fujimoto, Masa-Katsu, Fujita, Ryuichi, Fukushima, Mitsuhiro, Futamase, Toshifumi, Harada, Tomohiro, Hashimoto, Tatsuaki, Hayama, Kazuhiro, Hikida, Wataru, Himemoto, Yoshiaki, Hirabayashi, Hisashi, Hiramatsu, Takashi, Horisawa, Hideyuki, Hosokawa, Mizuhiko, Ishikawa, Takehiko, Kawano, Isao, Koizumi, Hiroyuki, Kuninaka, Hitoshi, Matsuhara, Hideo, Morimoto, Mutsuko Y., Nishiyama, Kazutaka, Sakai, Shin-ichiro, Takahashi, Tadayuki, and Utashima, Masayoshi

Subjects
Physics, Optics, Physics and Astronomy (miscellaneous), Gravitational wave, business.industry, Big Bang Observer, Antenna (radio), Space (mathematics), business
Abstract

著者人数: 145名, 資料番号: SA1002921000

Published
2011
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