Home > Publications database > Measurement of the thermal accommodation coefficient of helium on a crystalline silicon surface at low-temperatures |
Journal Article | PUBDB-2024-08006 |
; ; ; ; ; ; ;
2024
IOP Publ.
Bristol
This record in other databases:
Please use a persistent id in citations: doi:10.1088/1361-6382/ad7184 doi:10.3204/PUBDB-2024-08006
Report No.: arXiv:2402.11977
Abstract: Proposals for next-generation gravitational wave observatories include cryogenically cooled 200 kg test mass mirrors suspended from pendulums and made of 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 $\alpha(11\,\mathrm{K} \lt T \lt 30\,\mathrm{K})$, which is the probability that a helium atom thermalises with a surface at a given temperature when reflected from it. We find $\alpha(T) \gt 0.7$ for temperatures ${\lt}20$ 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.
![]() |
The record appears in these collections: |
Preprint
Measurement of the thermal accommodation coefficient of helium on a crystalline silicon surface at low-temperatures
Files
Fulltext by arXiv.org
BibTeX |
EndNote:
XML,
Text |
RIS