We present results of experiments into the stabilization of the amplitude of Nd:YAG lasers for use in advanced gravitational wave detectors. By feeding back directly to the pump-diode driving current we achieved shot-noise-limited stabilization at frequencies up to several kHz with some residual noise at lower frequencies (sub ~100 Hz). The method used is applicable to higher powered laser systems planned for advanced interferometric gravitational wave detectors
The output power of a cw Nd:YAG laser was stabilized in a dc-coupled feedback loop with a low-noise ...
Second-generation interferometric gravitational wave detectors require high-power lasers with approx...
Second generation gravitational wave detectors require high power lasers with more than 100 W of out...
We present results on the power stabilization of a Nd:YAG laser in the frequency band from 1 Hz to 1...
We present results on the power stabilization of a Nd:YAG laser in the frequency band from 1 Hz to 1...
We present results on the power stabilization of a Nd:YAG laser in the frequency band from 1 Hz to 1...
Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.Includes bibliographica...
The output power of a cw Nd:YAG laser was stabilized in a dc-coupled feedback loop with a low-noise ...
The output power of a cw Nd:YAG laser was stabilized in a dc-coupled feedback loop with a low-noise ...
Second generation gravitational wave detectors require high power lasers with more than 100 W of out...
Many experiments in modern physics set highly demanding requirements on their laser light sources. P...
Second generation gravitational wave detectors require high power lasers with more than 100 W of out...
Many experiments in modern physics set highly demanding requirements on their laser light sources. P...
Second generation gravitational wave detectors require high power lasers with several 100W of output...
Second generation gravitational wave detectors require high power lasers with several 100W of output...
The output power of a cw Nd:YAG laser was stabilized in a dc-coupled feedback loop with a low-noise ...
Second-generation interferometric gravitational wave detectors require high-power lasers with approx...
Second generation gravitational wave detectors require high power lasers with more than 100 W of out...
We present results on the power stabilization of a Nd:YAG laser in the frequency band from 1 Hz to 1...
We present results on the power stabilization of a Nd:YAG laser in the frequency band from 1 Hz to 1...
We present results on the power stabilization of a Nd:YAG laser in the frequency band from 1 Hz to 1...
Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.Includes bibliographica...
The output power of a cw Nd:YAG laser was stabilized in a dc-coupled feedback loop with a low-noise ...
The output power of a cw Nd:YAG laser was stabilized in a dc-coupled feedback loop with a low-noise ...
Second generation gravitational wave detectors require high power lasers with more than 100 W of out...
Many experiments in modern physics set highly demanding requirements on their laser light sources. P...
Second generation gravitational wave detectors require high power lasers with more than 100 W of out...
Many experiments in modern physics set highly demanding requirements on their laser light sources. P...
Second generation gravitational wave detectors require high power lasers with several 100W of output...
Second generation gravitational wave detectors require high power lasers with several 100W of output...
The output power of a cw Nd:YAG laser was stabilized in a dc-coupled feedback loop with a low-noise ...
Second-generation interferometric gravitational wave detectors require high-power lasers with approx...
Second generation gravitational wave detectors require high power lasers with more than 100 W of out...