Bøger af Lutz Winkelmann

One approach to detect gravitational waves, which have been postulated by Albert Einstein in his General Theory of Relativity, is based on interferometric measurements oflength variations with a large-scale Michelson interferometer. The detection range of theseground-based observatories is currently limited to approx. 15 Megaparsec (Mpc) becauseof a reduced sensitivity at detection frequencies of 10 Hz ¿ 10 kHz by shot noise. Theselimitations can be overcome by an output power increase of the detector¿s light source,which will enhance the sensitivity by an order of magnitude. Thus, the possibility of detecting a gravitational wave will be raised by a factor of 1000 and the detection range will be increased to 150 Mpc, accordingly.In this work a laser systems is presented, which fulfills the free-running laser requirementson stability and beam quality required by the next generation of gravitational wave detectors for the first time. The developed laser system is based on a two-stage concept,supplemented with an active amplitude and frequency stabilization, which is not partof this work. A 35 W Nd:YVO4 amplifier system with an emission wavelength of 1064nm represents the frequency reference of the laser system and is used as the seed for aninjection-locked high power oscillator. This amplifier, which is based on a Master OscillatorPower Amplifier scheme, is already used in today¿s gravitational wave detectors and hasbeen proven to be reliable in long-term operation. The linearly polarized output power ofmore than 200 W is generated inside the oscillator stage, which consists of four Nd:YAGcrystals arranged in an asymmetric ring resonator configuration. To compensate for lossesdue to thermal birefringence inside the longitudinally pumped laser crystals, an imagingdepolarization compensation is used.