Image Details
Caption: Figure 1.
(a) Equilibrium C–N bond lengths (in angstroms) of HMT+ in the calculated stable conformers with C3v (blue) and C2v (black) symmetry. The C3v structure is slightly more stable than the C2v structure, with a small barrier of 14.6 kJ mol–1 before zero-point energy correction. (b) NTO pairs representing the D3←D0 transition for both optimized D0 structures (C3v, C2v).
© 2026. The Author(s). Published by the American Astronomical Society.