Articles you may be interested inFeasibility of characterizing laser-ablated carbon plasmas via planar laser induced fluorescencea) Rev. Sci. Instrum. 83, 10E515 (2012); 10.1063/1.4733562Spatio-temporal mapping of ablated species in ultrafast laser-produced graphite plasmas Growth and structure of fullerene-like CN x thin films produced by pulsed laser ablation of graphite in nitrogen Chemistry, energy, and spatial distributions of species in carbon-nitrogen plasma plumes were investigated to define plasma conditions for growth of carbon nitride CN x films with a fullerene-like structure. Plumes were generated by ablation of graphite using a 248 nm excimer laser in the presence of low-pressure nitrogen. The plumes were investigated using element specific imaging, time-of-flight experiments, fluorescence spectroscopy, and molecular vibration sequence analyses. Studies showed the importance of plume/substrate interaction in causing secondary excitation phenomena. For N 2 pressures within the 5-50 mTorr range, plasmas at the substrate vicinity were found to consist mostly of atomic carbon, CN and C 2 molecules. Kinetic energies were calculated within 10-20 eV for mono atomic carbon, 30-55 eV for CN, and 20-40 eV for C 2 . Excited CN and C 2 molecules were generated by laser ablation and by collisions of the plume with the substrate surface. Their vibrational energies were strongly influenced by nitrogen pressure and time after a laser pulse. For pressures below 30 mTorr, vibrational energy was as high as 4.0 eV at 2-4 s for CN and 2.5 eV at 8 -10 s for C 2 . This low pressure was suggested for the growth of fullerene-like CN x films based on correlations between plasma parameters and film composition and bonding. Synthesis of the fullerene-like structure required high molecular temperatures at the condensation surface. High concentrations of CN radicals in the plasma promoted nitrogen incorporation into the films. Correlations among CN x film composition/bonding, excitation maximums, and kinetic/ vibrational energies of atomic carbon, CN and C 2 species located near the condensation surface are discussed.