This paper presents a theoretical investigation into the nature of the Au-bearing states immediately preceding transient Au–H chemistry in post-r-process kilonova ejecta. Conventional models implicitly assume that gold synthesized via the r-process exists as isolated monatomic Au before interacting with hydrogen. However, the 2025 SLAC/European XFEL synthesis of Au₂Hₓ under extreme pressure and temperature, using hydrocarbon-derived hydrogen, suggests that Au–H chemistry need not proceed through simple binary association of bare Au and free H. This paper formulates the Au-bearing precursor problem: was the Au-bearing state immediately preceding any transient gold hydride chemistry truly elemental gold, or a more complex intermediate? This question is positioned not as a challenge to r-process nucleosynthesis theory, but as a new research question in post-nucleosynthetic astrochemistry, tractable through future DFT calculations, laboratory experiments, and spectroscopic observation.
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