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Space gravitational-wave antennas DECIGO and B-DECIGO

Kawamura, Seiji and Arai, Koji (2019) Space gravitational-wave antennas DECIGO and B-DECIGO. International Journal of Modern Physics D, 28 (12). Art. No. 1845001. ISSN 0218-2718. https://resolver.caltech.edu/CaltechAUTHORS:20191017-141101754

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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.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1142/s0218271818450013DOIArticle
ORCID:
AuthorORCID
Arai, Koji0000-0001-8916-8915
Additional Information:© 2019 World Scientific Publishing Co Pte Ltd. Received 1 April 2018; Accepted 2 May 2018; Published: 4 June 2018.
Group:LIGO
Subject Keywords:Gravitational-wave; inflation; Fabry–Perot Michelson interferometer; multimessenger astronomy
Issue or Number:12
Classification Code:PACS: 04.80.Nn, 95.55.Ym, 95.85.Sz, 07.60.Ly
Record Number:CaltechAUTHORS:20191017-141101754
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191017-141101754
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:99333
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:19 Oct 2019 04:44
Last Modified:19 Oct 2019 04:44

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