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Cited by 423

The DOI matches its Crossref record; 22 of the 22 references it cites were found in a registry or an index.

Current status of space gravitational wave antenna DECIGO and B-DECIGO

Open access
Kawamura, Seiji, Ando, Masaki, Seto, Naoki, Sato, Shuichi, Musha, Mitsuru, Kawano, Isao, Yokoyama, Jun’ichi, Tanaka, Takahiro, Ioka, Kunihito, Akutsu, Tomotada, Takashima, Takeshi, Agatsuma, Kazuhiro, Araya, Akito, Aritomi, Naoki, Asada, Hideki, Chiba, Takeshi, Eguchi, Satoshi, Enoki, Motohiro, Fujimoto, Masa-Katsu, Fujita, Ryuichi, Futamase, Toshifumi, Harada, Tomohiro, Hayama, Kazuhiro, Himemoto, Yoshiaki, Hiramatsu, Takashi, Hong, Feng-Lei, Hosokawa, Mizuhiko, Ichiki, Kiyotomo, Ikari, Satoshi, Ishihara, Hideki, Ishikawa, Tomohiro, Itoh, Yousuke, Ito, Takahiro, Iwaguchi, Shoki, Izumi, Kiwamu, Kanda, Nobuyuki, Kanemura, Shinya, Kawazoe, Fumiko, Kobayashi, Shiho, Kohri, Kazunori, Kojima, Yasufumi, Kokeyama, Keiko, Kotake, Kei, Kuroyanagi, Sachiko, Maeda, Kei-ichi, Matsushita, Shuhei, Michimura, Yuta, Morimoto, Taigen, Mukohyama, Shinji, Nagano, Koji, Nagano, Shigeo, Naito, Takeo, Nakamura, Kouji, Nakamura, Takashi, Nakano, Hiroyuki, Nakao, Kenichi, Nakasuka, Shinichi, Nakayama, Yoshinori, Nakazawa, Kazuhiro, Nishizawa, Atsushi, Ohkawa, Masashi, Oohara, Kenichi, Sago, Norichika, Saijo, Motoyuki, Sakagami, Masaaki, Sakai, Shin-ichiro, Sato, Takashi, Shibata, Masaru, Shinkai, Hisaaki, Shoda, Ayaka, Somiya, Kentaro, Sotani, Hajime, Takahashi, Ryutaro, Takahashi, Hirotaka, Akiteru, Takamori, Taniguchi, Keisuke, Taruya, Atsushi, Tsubono, Kimio, Tsujikawa, Shinji, Ueda, Akitoshi, Ueda, Ken-ichi, Watanabe, Izumi, Yagi, Kent, Yamada, Rika, Yokoyama, Shuichiro, Yoo, Chul-Moon, Zhu, Zong-Hong·2021·Progress of Theoretical and Experimental Physics
DOI 10.1093/ptep/ptab019
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Abstract

The Deci-hertz Interferometer Gravitational Wave Observatory (DECIGO) is a future Japanese space mission with a frequency band of 0.1 Hz to 10 Hz. DECIGO aims at the detection of primordial gravitational waves, which could have been produced during the inflationary period right after the birth of the Universe. There are many other scientific objectives of DECIGO, including the direct measurement of the acceleration of the expansion of the Universe, and reliable and accurate predictions of the timing and locations of neutron star/black hole binary coalescences. DECIGO consists of four clusters of observatories placed in heliocentric orbit. Each cluster consists of three spacecraft, which form three Fabry–Pérot Michelson interferometers with an arm length of 1000 km. Three DECIGO clusters will be placed far from each other, and the fourth will be placed in the same position as one of the other three to obtain correlation signals for the detection of primordial gravitational waves. We plan to launch B-DECIGO, which is a scientific pathfinder for DECIGO, before DECIGO in the 2030s to demonstrate the technologies required for DECIGO, as well as to obtain fruitful scientific results to further expand multi-messenger astronomy.

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Metadata

Authors
Kawamura, S., Ando, M., Seto, N., Sato, S., Musha, M., Kawano, I., Yokoyama, J., Tanaka, T., Ioka, K., Akutsu, T., Takashima, T., Agatsuma, K., Araya, A., Aritomi, N., Asada, H., Chiba, T., Eguchi, S., Enoki, M., Fujimoto, M.-K., Fujita, R., Futamase, T., Harada, T., Hayama, K., Himemoto, Y., Hiramatsu, T., Hong, F.-L., Hosokawa, M., Ichiki, K., Ikari, S., Ishihara, H., Ishikawa, T., Itoh, Y., Ito, T., Iwaguchi, S., Izumi, K., Kanda, N., Kanemura, S., Kawazoe, F., Kobayashi, S., Kohri, K., Kojima, Y., Kokeyama, K., Kotake, K., Kuroyanagi, S., Maeda, K.-I., Matsushita, S., Michimura, Y., Morimoto, T., Mukohyama, S., Nagano, K., Nagano, S., Naito, T., Nakamura, K., Nakamura, T., Nakano, H., Nakao, K., Nakasuka, S., Nakayama, Y., Nakazawa, K., Nishizawa, A., Ohkawa, M., Oohara, K., Sago, N., Saijo, M., Sakagami, M., Sakai, S.-I., Sato, T., Shibata, M., Shinkai, H., Shoda, A., Somiya, K., Sotani, H., Takahashi, R., Takahashi, H., Akiteru, T., Taniguchi, K., Taruya, A., Tsubono, K., Tsujikawa, S., Ueda, A., Ueda, K.-I., Watanabe, I., Yagi, K., Yamada, R., Yokoyama, S., Yoo, C.-M., & Zhu, Z.-H.
Venue
Progress of Theoretical and Experimental Physics
Publisher
Oxford University Press (OUP)
Published
2021-02-22
Volume
2021
Issue
5
ISSN
2050-3911 (ISSN-L)
DOI
10.1093/ptep/ptab019
OpenAlex
W3131530517
Cited by
423
References
22
FWCI
34.19
Type
journal article
Language
en
Open access
gold

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CoChat. (2026). Citation check: Current status of space gravitational wave antenna DECIGO and B-DECIGO. https://app.cochat.ai/papers/10.1093/ptep/ptab019
The paper
Kawamura, S., Ando, M., Seto, N., Sato, S., Musha, M., Kawano, I., Yokoyama, J., Tanaka, T., Ioka, K., Akutsu, T., Takashima, T., Agatsuma, K., Araya, A., Aritomi, N., Asada, H., Chiba, T., Eguchi, S., Enoki, M., Fujimoto, M.-K., . . . Zhu, Z.-H. (2021). Current status of space gravitational wave antenna DECIGO and B-DECIGO. Progress of Theoretical and Experimental Physics. https://doi.org/10.1093/ptep/ptab019

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.