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arXiv · 2310.01709

Investigation of flow patterns in two-phase carbon dioxide in horizontal and vertical pipes

Alexander Siegfanz·Wolfgang Wagner·Uwe Janoske
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Abstract

Modern particle detectors crucially depend on efficient cooling systems. Two-phase carbon dioxide (CO$_2$) is a suitable solution as a cooling agent. This publication presents the observations and results of investigations of horizontal and vertical flow of two-phase CO$_2$ at a temperature of $T=-15\,^\circ$C and a pressure of approximately $23\,$bar. Heat fluxes between $98.5\,$kW/m$^2$ and $200\,$kW/m$^2$ were applied to the CO$_2$, covering the range expected to occur in the future ATLAS Pixel detector being built for the high-luminosity phase of the Large Hadron Collider. Flow speeds ranged from $11.8\,$m/s to $28.1\,$m/s. Dedicated sensors were used to measure the temperature and pressure before and after heating the CO$_2$. Two-phase flow patterns occuring in the pipe after heating the CO$_2$ were recorded with a high-speed camera. Stratified, wavy and slug flow are found to be the predominant patterns for horizontal flow, while upward vertical flow is mainly found to be slug or churn. Based on the recorded images the void fraction of the CO$_2$ after heating is determined and compared for the different setups. The results are summarised in a flow-pattern map. A clear distinction between vertical and horizontal flow is found, with horizontal flow exhibiting a significantly higher void fraction than vertical flow. Based on the pressure measurements, the pressure drop after heating the CO$_2$ is measured and the corresponding Euler number is computed. While the pressure drop increases with the heat flux for horizontal flow due to frictional losses, the pressure drop reduces with the heat flux in case of upward vertical flow, since static pressure is important in this case.

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Alexander Siegfanz, Wolfgang Wagner, Uwe Janoske. 2023-10-03. Investigation of flow patterns in two-phase carbon dioxide in horizontal and vertical pipes. https://arxiv.org/abs/2310.01709

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