Study of selected mild steels for application in vacuum systems of future gravitational wave detectors
Carlo Scarcia, Giuseppe Bregliozzi, Paolo Chiggiato, Alice, Ingrid Michet, Ana Teresa Perez Fontenla, Martino Rimoldi, Mauro, Taborelli, Ivo Wevers

TL;DR
This study evaluates mild steel as a cost-effective alternative to stainless steel for vacuum systems in future gravitational wave detectors, focusing on outgassing behavior and surface chemistry after low-temperature bakeouts.
Contribution
It demonstrates that mild steel has significantly lower hydrogen outgassing rates and maintains surface properties after repeated bakeouts and air exposure, making it suitable for GWD vacuum systems.
Findings
Mild steel exhibits hydrogen outgassing below 10^{-14} mbar l s^{-1} cm^{-2} after bakeouts.
Repeated low-temperature bakeouts reduce water vapor outgassing.
Surface conditions of mild steel remain stable after six months of air exposure.
Abstract
Next-generation gravitational wave detectors (GWDs) like the Cosmic Explorer and Einstein Telescope require extensive vacuum tubing, necessitating cost-effective materials. This study explores the viability of mild steel as an alternative to austenitic stainless steel for UHV beampipes, focusing on outgassing rates and surface chemistry after low-temperature bakeouts. Mild steels exhibit significantly lower hydrogen outgassing rates, below 10 mbar l s cm after bakeouts at 80{\deg}C for 48 hours. While water vapor is the primary residual gas after such low-temperature bakeouts, repeated treatments reduce its outgassing rate and modify surface conditions so that such benefit is preserved after at least six months of exposure to laboratory air. These findings position mild steel as an economical and efficient material for future GWD beampipes.
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