Physics
Scientific paper
Apr 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cqgra..23s.287m&link_type=abstract
Classical and Quantum Gravity, Volume 23, Issue 8, pp. S287-S292 (2006).
Physics
Scientific paper
We have developed a fibre-MOPA (master oscillator power amplifier) system as the light source of the future gravitational wave detectors. The output power from a 500 mW NPRO emitting 1064 nm was amplified by an Yb-doped double-clad fibre amplifier, and the maximum output power and the optical optical conversion efficiency were 12 W and 89%, respectively. The diffraction-limited beam was obtained from the multi-mode fibre amplifier by bending the fibre. The frequency noise and intensity noise of the fibre-MOPA were evaluated and suppressed.
Miura Jun-ichi
Musha Mitsuru
Nakagawa Ken'ichi
Ueda Ken-ichi
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