D3+ formation through photoionization of the molecular D2-D2 dimer

The H-2-H-2 molecular dimer is of fundamental importance in the study of chemical interactions because of its unique bonding properties and its ability to model more complex systems. The trihydrogen cation H-3(+) is also a key intermediate in a range of chemical processes in interstellar environments, such as the formation of various organic molecules and early stars. However, the unexpected high abundance of H-3(+) in molecular clouds remains challenging to explain. Here using near-infrared, femtosecond laser pulses and coincidence momentum imaging, we find that the dominant channel after photoionization of a deuterium molecular dimer (D-2-D-2) is the ejection of a deuterium atom within a few hundred femtoseconds, leading to the formation of D-3(+). The formation mechanism is supported and well-reproduced by ab initio molecular dynamics simulations. This pathway of D-3(+) formation from ultracold D-2-D-2 gas may provide insights into the high abundance of H-3(+) in the interstellar medium.

Automated summary

Using near-infrared, femtosecond laser pulses and coincidence momentum imaging, it is found that the dominant channel after photoionization of a deuterium molecular dimer (D-2-D-2) is the ejection of a deuterium atom within a few hundred femtoseconds, leading to the formation of D-3(+). This pathway of D-3(+) formation from ultracold D-2-D-2 gas may provide insights into the high abundance of H-3(+) in the interstellar medium.