High-power Laser Systems

High-power Laser Systems

All currently operative interferometric gravitational-wave detectors use high-power lasers made in Hannover.

Stabilized lasers for advanced gravitational wave detectors

An AEI Hannover research team together with the Laser Zentrum Hannover e.V. has developed and provided pre-stabilized high-power laser systems to all currently operating large interferometric gravitational-wave detectors. Their experience gained by running earlier generations of theses systems at GEO600 was crucial to this success.

The Advanced LIGO laser system

The Albert Einstein Institute in Hannover carries subsystem responsibility for the Advanced LIGO 200 W pre-stabilized laser systems. In 2010-2012, AEI has provided, delivered and installed the laser systems both at the Hanford and Livingston observatory sites. The work on the PSL is split between the Laser Zentrum Hannover which concentrates on the laser development and the AEI which is in charge of diagnostic, control and stabilization of the high power laser system.

The aLIGO PSL consists of a 2 W Nd:YAG seed laser which is amplified via a Nd:YVO amplifier stage to 35 W. This 35 W laser serves as a master laser in an injection-locking scheme to seed a 200 W Nd:YAG high power oscillator stage. The output of the high power stage is spatially filtered by a newly developed bow-tie pre-mode cleaner (PMC) resonator which transmits 165 W in the fundamental Gaussian mode with only 1 % of the power in higher order modes. The PMC has two auxiliary ports to pick-off beam samples for the power and frequency stabilization. A diagnostic breadboard (DBB) is an integral part of the PSL and allows for a fully automated characterization of the 35 W and the 200 W laser with regard to temporal and spatial fluctuations and the spatial beam quality.

Since their installation the aLIGO PSLs operate stable and provide reliable light sources for the gravitational wave detectors.

In addition to the lasers at the LIGO site a copy of the 200 W PSL is operated in the AEI labs to evaluate the long-term performance of the system and to work on the optimization of system components. Furthermore the highly-stable 165 W laser beam is used in several experiments to generate high power beams at different wavelengths and with novel spatial beam profiles.

Relevant publications

Winkelmann, L.; Puncken, O.; Kluzik, R.; Veltkamp, C.; Kwee, P.; Poeld, J.; Bogan, C.; Willke, B.; Frede, M.; Neumann, J. et al.; Wessels, P.; Kracht, D.: Injection-locked single-frequency laser with an output power of 220 W. Applied Physics B: Lasers and Optics 102 (3), pp. 529 - 538 (2011)
Willke, B.: Stabilized lasers for advanced gravitational wave detectors. Laser & Photonics Reviews 4 (6), pp. 780 - 794 (2010)
Willke, B.; Danzmann, K.; Frede, M.; King, P.; Kracht, D.; Kwee, P.; Puncken, O.; Savage, Jr., R. L.; Schulz, B.; Seifert, F. et al.; Veltkamp, C.; Wagner, S.; Weßels, P.; Winkelmann, L.: Stabilized lasers for advanced gravitational wave detectors. 18th International Conference on General Relativity & Gravitation, Sydney, Australia, July 08, 2007 - July 13, 2007. Classical and Quantum Gravity 25 (11), 114040, (2008)
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