Journal Article PUBDB-2024-08006

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Measurement of the thermal accommodation coefficient of helium on a crystalline silicon surface at low-temperatures

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2024
IOP Publ. Bristol

Classical and quantum gravity 41(19), 195013 () [10.1088/1361-6382/ad7184]
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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.

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Note: 12 pages, 5 figures

Contributing Institute(s):
  1. Any Light Particle Search (ALPS)
Research Program(s):
  1. 611 - Fundamental Particles and Forces (POF4-611) (POF4-611)
  2. DFG project G:(GEPRIS)390833306 - EXC 2121: Quantum Universe (390833306) (390833306)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2024
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Measurement of the thermal accommodation coefficient of helium on a crystalline silicon surface at low-temperatures
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 Record created 2024-12-19, last modified 2025-07-23


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