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Frequency stabilization of a monolithic Nd:YAG ring laser by controlling the power of the laser-diode pump source

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

Brozek,  Oliver Sascha
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/persons40437

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

Quetschke,  Volker
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/persons40453

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

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Zitation

Willke, B., Brozek, O. S., Danzmann, K., Quetschke, V., & Gossler, S. (2000). Frequency stabilization of a monolithic Nd:YAG ring laser by controlling the power of the laser-diode pump source. Optics Letters, 25(14), 1019-1021. doi:10.1364/OL.25.001019.


Zitierlink: https://hdl.handle.net/11858/00-001M-0000-0013-570E-5
Zusammenfassung
The frequency of a 700-mW monolithic nonplanar Nd:YAG ring laser (NPRO) depends, with a large coupling coefficient (megahertz per milliwatt), on the power of its laser-diode pump source. Using this effect, we demonstrate frequency stabilization of a NPRO to a frequency reference by feeding back to the current of its pump diodes. We achieved an error-point frequency noise smaller than 1 mHz/root Hz and, simultaneously, a reduction of the power noise of the NPRO by 10 dB without an additional power-stabilization feedback syste