Abstract
Cations of diamondoids and derivatives thereof have recently become the subject of experimental, spectroscopic studies due to their potential role in astrochemistry. In particular, their electronic spectra and photoinduced dynamics trigger great interest. Here, we report on computational investigations of two nitrogen-containing derivatives of the adamantane cation (Ada+, C10H16+), the amantadine cation (Ama+, C10H15NH2+) and the cyanoadamantane cation (Ada-CN+, C10H15CN+). Specifically, we study electronic (vibrationally resolved) spectra and nonadiabatic molecular dynamics (modeled using the surface hopping approach based on semiempirical electronic structure theory) of these radical cations. The internal conversion time constants as well as reactive relaxation outcomes (cage-opening and hydrogen loss) are compared for the two derivatives and also with the case of Ada+ [Roy et al., Theor. Chem. Acc. 2023, 142, 71]. Remarkably, we find a longer ground-state recovery time for Ada-CN+ than for Ama+ (for the same excitation energy window), despite a smaller excitation energy for the former. Thus, a static energy gap law cannot be used to rationalize nonadiabatic dynamics and excited-state lifetimes in this case: Dynamics and details of the couplings between several states play a decisive role.
Supplementary materials
Title
SI: Nonadiabatic photodynamics of amantadine and cyanoadamantane cations: Departure form the energy gap law?
Description
Excitation energies, oscillator strengths, dominant orbital pairs for the amantadine and cyanoadamantane cations; populations for Ada-CN+ after excitation to the energy window of [3.5,5] eV; typical cage-opened structures of Ama+
Actions