Chemical models for simulating single-walled nanotube production in arc vaporization and laser ablation processes.
Chemical kinetic models for the nucleation and growth of clusters and single-walled carbon nanotube (SWNT) growth are developed for numerical simulations of the production of SWNTs. Two models that involve evaporation and condensation of carbon and metal catalysts, a full model involving all carbon clusters up to C80, and a reduced model are discussed. The full model is based on a fullerene model, but nickel and carbon/nickel cluster reactions are added to form SWNTs from soot and fullerenes. The full model has a large number of species--so large that to incorporate them into a flow field computation for simulating laser ablation and arc processes requires that they be simplified. The model is reduced by defining large clusters that represent many various sized clusters. Comparisons are given between these models for cases that may be applicable to arc and laser ablation production. Solutions to the system of chemical rate equations of these models for a ramped temperature profile show that production of various species, including SWNTs, agree to within about 50% for a fast ramp, and within 10% for a slower temperature decay time.
NASA Johnson Space Center, Houston, Texas, USA.
Carl D
CD
Scott
D002244:Carbon / Q000737:chemistry; D002384:Catalysis; D037741:Fullerenes / Q000737:chemistry; D007700:Kinetics; D007834:Lasers; D008956:Models, Chemical; D015233:Models, Statistical; D008962:Models, Theoretical; D037742:Nanotubes, Carbon / Q000737:chemistry*; D009532:Nickel / Q000737:chemistry; D012984:Software; D013696:Temperature; D013997:Time Factors
D037741:Fullerenes; D037742:Nanotubes, Carbon; D002244:Carbon; D009532:Nickel