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We reveal the microscopic vacancy trapping mechanism for H bubble formation in W based on first-principles calculations of the energetics of H-vacancy interaction and the kinetics of H segregation. Vacancy provides an isosurface of optimal charge density that induces collective H binding on its internal surface, a prerequisite for the formation of H₂ molecule and nucleation of H bubble inside the vacancy. The critical H density on the vacancy surface before the H₂ formation is found to be 10¹⁹--10²⁰ H atoms per m². We believe that such mechanism is generally applicable for H bubble formation in metals and metal alloys.
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Liu et al. (2009) studied this question.
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