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Birefringence in a Silicon Beamsplitter at 2um for Future Gravitational Wave Detectors
by
Adam, Alex
, Zhao, Chunnong
, Blair, Carl
in
Birefringence
/ Detectors
/ Float zones
/ Gravitational waves
/ Noise generation
/ Noise measurement
/ Noise sensitivity
/ Silicon substrates
/ Thermal noise
2024
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Birefringence in a Silicon Beamsplitter at 2um for Future Gravitational Wave Detectors
by
Adam, Alex
, Zhao, Chunnong
, Blair, Carl
in
Birefringence
/ Detectors
/ Float zones
/ Gravitational waves
/ Noise generation
/ Noise measurement
/ Noise sensitivity
/ Silicon substrates
/ Thermal noise
2024
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Birefringence in a Silicon Beamsplitter at 2um for Future Gravitational Wave Detectors
Paper
Birefringence in a Silicon Beamsplitter at 2um for Future Gravitational Wave Detectors
2024
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Overview
The next generation of gravitational wave detectors will move to cryogenic operation in order to reduce thermal noise and thermal distortion. This necessitates a change in mirror substrate with silicon being a good candidate. Birefringence is an effect that will degrade the sensitivity of a detector and is of greater concern in silicon due to its crystalline nature. We measure the birefringence in a float zone silicon beamsplitter since we expect there to be a large inherent birefringence due to the spatial dispersion effect. We observe that the birefringence varied between \\(3.44 \\pm 0.12 \\times 10^{-7}\\) and \\(1.63 \\pm 0.05 \\times 10^{-7}\\) and estimate the birefringence along the axis to be \\(1.64 \\pm 0.5 \\times 10^{-6}\\) at 2um. We demonstrate this effect and argue that it strengthens the case for 2um and silicon.
Publisher
Cornell University Library, arXiv.org
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