In liquid-helium refrigeration systems, seal failures or material outgassing can release trace amounts of hydrogen. The infiltration of hydrogen atoms into a metal’s crystal lattice can trigger hydrogen embrittlement, leading to reduced material plasticity and the initiation of cracks. For superconducting magnets operating over long periods within enclosed, low-temperature cavities containing trace hydrogen, the material's resistance to hydrogen embrittlement is a critical factor determining the long-term reliability of the components. Once hydrogen atoms enter the crystal lattice, they tend to accumulate at grain boundaries and dislocations, weakening the cohesive strength of the grain boundaries and facilitating crack formation under applied stress. Many niobium-based and tantalum-based refractory metals are highly susceptible to hydrogen absorption, making them prone to hydrogen embrittlement failure at both room and cryogenic temperatures. NbTi (niobium-titanium) alloy exhibits superior stability in hydrogen-containing environments compared to pure niobium; when compared with pure niobium, high-purity tantalum, molybdenum, tungsten, and the Ti6Al4V alloy, it demonstrates distinct characteristics under low-temperature, hydrogen-rich operating conditions.
Common engineering metals present significant drawbacks in low-temperature, hydrogen-containing environments. Carbon steel is highly susceptible to hydrogen embrittlement and is therefore unsuitable for use in cryogenic cavities. While 316L austenitic stainless steel offers moderate resistance to hydrogen embrittlement, its weak magnetic properties can interfere with magnetic fields. Copper and aluminum exhibit low hydrogen absorption but lack the mechanical strength required to withstand the prestress applied to magnets. Ti6Al4V titanium alloy readily absorbs hydrogen at room temperature to form hydrides; under low-temperature cyclic stress, these hydrides can induce crack formation, restricting its use to environments where hydrogen levels are strictly controlled. Conventional metals often suffer from either magnetic interference or a high risk of hydrogen embrittlement, making it difficult to simultaneously meet the requirements for non-magnetic properties, hydrogen embrittlement resistance, and cryogenic service.
This study provides a comparative analysis of the hydrogen absorption and hydrogen embrittlement behavior of pure niobium, high-purity tantalum, molybdenum, tungsten, and Ti6Al4V alloy. Pure niobium (Nb) is highly susceptible to hydrogen absorption; even a small amount of hydrogen can lead to the formation of niobium hydrides, causing the material to transition from a ductile state to a brittle one and resulting in rapid cracking under stress at low temperatures. High-purity tantalum (Ta) also exhibits a strong capacity for hydrogen absorption; the resulting hydrides significantly reduce the ductility of tantalum components, limiting their long-term service to environments with extremely low partial pressures of hydrogen. While metals like molybdenum (Mo) and tungsten (W) absorb little hydrogen at room temperature, they readily adsorb hydrogen during high-temperature degassing processes, which can lead to rapid hydrogen-induced crack propagation when subjected to stress at low temperatures. In Ti6Al4V titanium alloy, the formation of titanium hydrides—accompanied by volumetric expansion—generates persistent internal stress during thermal cycling, ultimately triggering cracks. In NbTi alloys, titanium is dissolved within the niobium matrix, which to some extent inhibits the continuous precipitation of hydrides; consequently, the threshold for hydrogen-induced brittle cracking is higher than that of pure niobium. However, this does not render NbTi entirely immune to hydrogen; if the partial pressure of hydrogen continues to rise, hydrides will still precipitate, leading to a degradation in superconducting performance.
Comparing different compositions of NbTi alloys, the Nb-47Ti variant demonstrates superior resistance to hydrogen embrittlement compared to alloys with higher niobium content. In high-niobium NbTi, the matrix more closely resembles pure niobium, resulting in a greater tendency to absorb hydrogen and a higher likelihood of hydrides forming continuous networks along grain boundaries. Conversely, in high-titanium NbTi, the increased titanium content facilitates the formation of titanium hydrides, raising the risk of localized stress concentration. The solid-solution structure of Nb-47Ti helps disperse hydrogen atoms, preventing the extensive, continuous precipitation of hydrides. In the environment of a cryogenic dewar—characterized by low temperatures and low hydrogen partial pressure—the degradation of the material's ductility and superconducting properties occurs very slowly. Nevertheless, in the event of a significant hydrogen leak, NbTi remains susceptible to damage from hydrogen embrittlement.
Currently, NbTi superconducting coils are well-established in conventional liquid-helium dewar systems; provided that vacuum integrity and degassing are properly controlled, the probability of failure due to hydrogen embrittlement is extremely low. The primary limitation of NbTi is its inability to withstand long-term service in extreme environments characterized by high hydrogen partial pressures or high hydrogen concentrations. Subsequently, surface passivation can be employed to block the ingress of hydrogen atoms, thereby enhancing the resistance of NbTi components to hydrogen-induced degradation and further increasing the safety margin of superconducting equipment in the event of a vacuum leak.
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