posted on 2023-07-05, 15:04authored byShane
J. Goettl, Lotefa B. Tuli, Andrew M. Turner, Yahaira Reyes, A. Hasan Howlader, Stanislaw F. Wnuk, Patrick Hemberger, Alexander M. Mebel, Ralf I. Kaiser
Molecular beam experiments together with electronic structure
calculations
provide the first evidence of a complex network of elementary gas-phase
reactions culminating in the bottom-up preparation of the 24π
aromatic coronene (C24H12) moleculea
representative peri-fused polycyclic aromatic hydrocarbon (PAH) central
to the complex chemistry of combustion systems and circumstellar envelopes
of carbon stars. The gas-phase synthesis of coronene proceeds via
aryl radical-mediated ring annulations through benzo[e]pyrene (C20H12) and benzo[ghi]perylene (C22H12) involving armchair-, zigzag-,
and arm-zig-edged aromatic intermediates, highlighting the chemical
diversity of molecular mass growth processes to polycyclic aromatic
hydrocarbons. The isomer-selective identification of five- to six-ringed
aromatics culminating with the detection of coronene is accomplished
through photoionization and is based upon photoionization efficiency
curves along with photoion mass-selected threshold photoelectron spectra,
providing a versatile concept of molecular mass growth processes via
aromatic and resonantly stabilized free radical intermediates to two-dimensional
carbonaceous nanostructures.