Abstract

We propose and experimentally demonstrate that the trihydrogen cation (H3+_3^+) can be produced via single photoionization of the molecular hydrogen dimer (H4_4). Using near-infrared, femtosecond laser pulses and coincidence momentum imaging, we find that the dominant channel after single ionization of the dimer is the ejection of a hydrogen atom within a few hundred femtoseconds, leaving an H3+ cation behind. The formation mechanism is supported and well reproduced by an ab-initio molecular dynamics simulation. This is a new pathway of H3+_3^+ formation from ultracold hydrogen gas that may help explain the unexpected high abundance of H3+_3^+ in the interstellar medium in the universe.

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