Open Access Paper
25 September 2017 Developments of highly frequency and intensity stabilized lasers for space gravitational wave detector decigo/pre-decigo
Ken'ichi Nakagawa, Ayumi Shimo-oku, Ken'ichi Nakagawa, Mitsuru Musha
Author Affiliations +
Proceedings Volume 10562, International Conference on Space Optics — ICSO 2016; 105620H (2017) https://doi.org/10.1117/12.2296057
Event: International Conference on Space Optics — ICSO 2016, 2016, Biarritz, France
Abstract
Gravitational wave (GW), predicted by A. Einstein in his general theory of relativity, is temporal variation of spatial distortion caused from the change of enormous mass such as inspiral and merger of neutron star binaries, black hole binaries, explosion of supernovae, and inflation in early universe.
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Ken'ichi Nakagawa, Ayumi Shimo-oku, Ken'ichi Nakagawa, and Mitsuru Musha "Developments of highly frequency and intensity stabilized lasers for space gravitational wave detector decigo/pre-decigo", Proc. SPIE 10562, International Conference on Space Optics — ICSO 2016, 105620H (25 September 2017); https://doi.org/10.1117/12.2296057
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KEYWORDS
Laser stabilization

Signal detection

Light sources

Interference (communication)

Fiber lasers

Servomechanisms

Bragg cells

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