The GEO 600 laser system

Zawischa, I.; Brendel, Martina; Danzmann, Karsten; Fallnich, Carsten; Heurs, Michele; Nagano, S.; Quetschke, Volker; Welling, H.; Willke, Benno

doi:10.1088/0264-9381/19/7/374

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The GEO 600 laser system

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Danzmann, Karsten
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

Nagano, S.
AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;
AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons40511

Willke, Benno
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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引用

Zawischa, I., Brendel, M., Danzmann, K., Fallnich, C., Heurs, M., Nagano, S., Quetschke, V., Welling, H., & Willke, B. (2002). The GEO 600 laser system. Classical and Quantum Gravity, 19(7), 1775-1781. doi:10.1088/0264-9381/19/7/374.

引用: https://hdl.handle.net/11858/00-001M-0000-0013-53B3-4

要旨

Interferometric gravitational wave detectors require high optical power, single frequency lasers with very good beam quality and high amplitude and frequency stability as well as high long-term reliability as input light source. For GEO 600 a laser system with these properties is realized by a stable planar, longitudinally pumped 12 W Nd:YAG rod laser which is injection-locked to a monolithic 800 mW Nd:YAG non-planar ring oscillator. Frequency control signals from the mode cleaners are fed to the actuators of the non-planar ring oscillator which determines the frequency stability of the system. The system power stabilization acts on the slave laser pump diodes which have the largest influence on the output power. In order to gain more output power, a combined Nd:YAGNd:YVO4 system is scaled to more than 22 W.