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Proceedings Paper • Open Access

Japanese space gravitational wave antenna DECIGO and DPF
Author(s): Mitsuru Musha

Paper Abstract

The gravitational wave detection will open a new gravitational wave astronomy, which gives a fruitful insight about early universe or birth and death of stars. In order to detect gravitational wave, we planed a space gravitational wave detector, DECIGO (DECi-heltz Interferometer Gravitational wave Observatory), which consists of three drag-free satellites forming triangle shaped Fabry-Perot laser interferometer with the arm length of 1000 km, and whose strain sensitivity is designed to be 2x10-24 /√Hz around 0.1 Hz. Before launching DECIGO around 2030, a milestone mission named DECIGO pathfinder (DPF) is planed to be launched whose main purpose is the feasibility test of the key technologies for DECIGO. In the present paper, the conceptual design and current status of DECIGO and DPF are reviewed.

Paper Details

Date Published: 17 November 2017
PDF: 6 pages
Proc. SPIE 10563, International Conference on Space Optics — ICSO 2014, 105632J (17 November 2017); doi: 10.1117/12.2304208
Show Author Affiliations
Mitsuru Musha, Univ. of Electro-Communications (Japan)


Published in SPIE Proceedings Vol. 10563:
International Conference on Space Optics — ICSO 2014
Zoran Sodnik; Bruno Cugny; Nikos Karafolas, Editor(s)

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