arXiv · 2402.11977
Measurement of the thermal accommodation coefficient of helium on a crystalline silicon surface at low-temperatures
Abstract
Next-generation gravitational wave observatories are expected to use cryogenically cooled, pendulum-suspended 200 kg test mass mirrors from a crystalline material such as crystalline silicon. During operation of the observatories, these mirrors undergo heating due to the absorption of laser radiation of up to a watt. Low noise cooling techniques need to be developed. Low-pressure helium exchange gas at 5 K might contribute to the challenging task. Here, we report the measurement of the helium accommodation coefficient $\alpha(11\,\mathrm{K} 0.7$ for temperatures < 20 K, which increases the cooling power compared to recently used assumptions. The idea of free molecular flow helium gas cooling is thus supported and might find application in some observatory concepts.
Explore related subjects
Keep this discovery
Alexander Franke, Nils Sültmann, Christoph Reinhardt, Sandy Croatto, Jörn Schaffran, Hossein Masalehdan, Axel Lindner, Roman Schnabel. 2024-02-19. Measurement of the thermal accommodation coefficient of helium on a crystalline silicon surface at low-temperatures. https://arxiv.org/abs/2402.11977
Cite the original work for its findings. Save a collection to share your selection of sources.