by
Xinlei Hua, Tahir Cagin, Jianwei Che and William A. Goddard III
aMaterials and Process Simulation Center,
California Institute of Technology,
Pasadena, California, 91125
E-mail: tahir@wag.caltech.edu
This is a draft paper for the
Seventh
Foresight Conference on Molecular Nanotechnology.
[Optional, if also separately submitted for journal peer review] The final version has been submitted
for publication in the special Conference issue of Nanotechnology.
One of the most puzzling aspects of fullerenes is how such complicated symmetric molecules are formed from a gas of atomic carbons, namely, the atomistic or chemical mechanisms. Are the atoms added one by one or as molecules (C2, C3)? Is there a critical nucleus beyond which formation proceeds at gas kinetic rates? What determines the balance between forming buckyballs, buckytubes, graphite and soot? The answer to these questions is extremely important in manipulating the systems to achieve particular products. A difficulty in current experiments is that the products can only be detected on time scales of microseconds long after many of the important formation steps have been completed. Consequently, it is necessary to use simulations, quantum mechanics and molecular dynamics, to determine these initial states. Experiments serve to provide the boundary conditions that severely limit the Using quantum mechanical methods (DFT) we derived a force field (MSXX FF) to describe one-dimensional (rings) and two-dimensional (fullerene) carbon molecules. Combining DFT with the MSXX FF, we calculated the energetics for the ring fusion spiral zipper (RFSZ) mechanism for formation of C60 fullerenes. Our results shows that the RFSZ mechanism is consistent with the quantum mechanics (with a slight modification for some of the intermediates).
One of the most puzzling aspects of fullerenes (C60, C70, etc.) is how such complicated symmetric molecules are formed from a gas of atomic carbons [atomcarbon], namely, the atomistic or chemical mechanism. Are the atoms added one by one or as molecules (C2, C3)? Is the C60 fullerene formed by adding C1, C2, or C3 to some smaller fullerene or is C60 formed by isomerization of some type of precursor molecule C60? Is there a critical nucleus beyond which formation proceeds at gas kinetic reates? What determines the balance bwtween forming buckyballs, buckytubes, graphite, and soot? The answer to these questions might lead to means of manipulating the systems to achieve particular products.
A difficulty in current experiments [Jarrold 1993, Jarrold 1994, Bowers 1993a, 1993b] is that the products can only be detected on times scales of $\mu$s, long after many of the important formation steps have been completed. Consequently, it is necessary to use first principles quantum mechanical theory to determine these initial states; however, the experiments serve to provide boundary condition that severely limint the possibilities, making the use of first principles theory practicable.
We selected density functinal theory (DFT) as the best compromise between accuracy and speed for studying these systems. We use the Becke gradient corrected exchange and the gradient corrected correlation functional of Lee, Yang, and Parr. [Johnson 1993] The calculations were carried out using PS-GVB with the 6-31G* basis set [Rignalda 1995].
Because the carbon rings play a central role, we studied how the structures and energetics of such rings changed with size and extracted a force field (denoted as the MSX FF) that would reproduce the DFT energetics and structures. This MSX FF would be used later in conjunction with the DFT calculations on various multiring systems to estimate the energetics of the full 60 atom systems without the necessity of DFT on the complete system.
The calculations on ring systems up to C60 are shown in Figure 1. The energies quoted here are cohesive energy par carbon atom. In calculating these energies we used as our reference the triplet C atom, calculated by LSDA.
C4m+2 is more stable than C4m. But as n --> infinity, the difference in Ecoh decreases to zero, leading to Einfinitysp1=6.56eV.
Both the polyacetylene and polyallene structures involve sigma-bonds that are sp1 hybrids, which prefer linear geometries. Thus we expect a strain energy proportional to
Indeed we found strain energy increase linearly with 1/n2 with slopes of 63.3 eV/n2 for 4m and 40.1eV/n2 for the 4m+2, respectively. Both converg to Einfinitysp1=6.56eV$
The force field took the following form:
Here qr1(l)=Ri(l)-Ri0(l)$ is the bond strain term, where for n=4m, i=1 is the triple bond and i=2 is the single bonds; for n=4m+2 their bonds are equivalent. The angle strain term is qtheta(l)=theta(l)-theta0(l) We use the periodic boundary condition so that, with theta0 = pi, n/2+1=1, where n is the total number of atoms in the system and n/2 is the number of unit cells. E0 is a reference energy corresponding to zero strain energy structure. (infinite linear chain) Comparing EMSX with EDFT for several structures, we can derive the force field parameters.
In a simular fasion we can derive the force field for the sp2 bonded carbons. The optimum structure for bulk carbon is graphite, which has each carbon bonded to three others (sp2 bonding) to form hexagonal sheets stacked on each other. The fullerenes structures can be considered as finite two dimensional anologs, in which each carbon is distorted (strained) from its preferred planar configuration. Since the strain should be proportinal to the square of the planar distortion angle, delta psi, we expect that the strain energy should scale as 1/n
We have performed the DFT(Becke/LYP) calculations on Cn fullerenes with n=20, 32 and 60. Figure 1 shows the cohesive energies per carbon atom.
Extrapolating the calculated cohesive energy to n ---> infinity leads to a cohesive energy per sp2 carbon of Ecohsp2 = 7.71 eV. This can be compared to the experimental cohesive energy of a single graphitic sheet of Esheetcoh=7.74eV. This is derived from the experimental cohesive energy [CRC Handbook] of graphite of Egraphite=7.8eV plus total Van der Waals attraction of Evdw=0.056eV between sheets calculated using the graphite force field. [Guo 1992]
Now that we have the energy and force field of both sp1 and sp2 hybridized carbon we can get the energetics of any carbon clusters. Adding the entropic controbution within harmonic approximation using FF, we get the free energy of various species at different temperature, which dictate the thermal equilibrium distribution of these species. Our population analysis is shown in Figure 2.

For studying formation reaction sequence we adopt two level of models, a fine one and a coarse one, as explained below.
We extend the MSX FF to include terms capable of describing the different bonding schemes. The key components are the additive energy terms for the dangling bond and the energy cost for bending a triple bond to form a 1,2-benzyne. Our FF are defined as follows:
We have chosen E0=60 epsilon1, as zero point. Here, n2 is the sp2 bonded carbons, n2 (epsilon1 - epsilon2) gives the energy gained by converting sp1 bonded carbon into spn2 bonded carbon, with epsilon1=-6.56eV$ and epsilon2=-7.71 eV. d1 is the energy of a dangling bond relative to the sigma-bonded state, nR number of of such dangling bond(radicals); d2 is the energy of an atom participating bended planar pi-bond relative to the sigma-bonded state and nsigma pi is the number of such atoms. We use the Benson-like scheme to evaluate d1 and d2 [Guo 1992] and found d1=2.32eV and d2=1.64eV. Estr (n2) is the strain energy and it is evaluated at the minimum energy structure.
We would use the fine model for the initial steps in the $C_{60}$ formation. As the reaction take off and begin to release more and more energy, we switch to the coase one.
At the beginning atomic carbons combine themselves to form dimers and trimer, C2, C3. These would then grow into linear chain of carbons Cn, etc., for n<10. [Hutter 1994] When n>10 the carbon cluster prefer ring structure [Hutter 1994] because beyond n>10 the energy gain in killing the dangling bonds at the two ends over compensate for the strain energy incured by folding up the chain. At around n>30 the ring structures give way to fullerene structures,[Bowers 1993a, 1993b] because replacing more pi-bond by sigma-bond over compensate for the strain of folding the 2-D net.
One process of C60 formation, as suggested by Jarrolds experiments, [Bowers 1993a, 1993b, Jarrold 1994] is to combine two C30 rings to form a bycyclic C60 ring, which in turn isomerized into a C60 fullerene. This unimolecular reaction will be the focus of our study.
As a mnemonic for referring to the various structures, we will simply denote the ring sizes of a structure. Thus the simple C60 ring is denoted as 60, while the double ring system, 1, is 30+4+30. This notation does not uniquely describe a structure, but it is for the species we will consider. We will take the reference energy to be Eo=60 epsilon1, where epsilon1=-6.56eV.
Following Jarrold, the first few steps in the reaction are as follows: (see Figure 4)

The driving force for the growth is the gain in forming sp2 sigma bond. The opposing forces are the energy lost by the radicals created along the way and the increasing strain energies.
The Jarrold mechanism represents an innovative major step forward in understanding the formation of C60 fullerene. Our energetic analysis shows that some of the reactions pathways have large energy barriers, however they never exceed the energy available to the unimolecular reaction.
The similar approach could be used to study the formation of other fullerenes, like C40, C50, C70, etc..
Why C60 is so stable and how C60 fullerenes are formed, these are the two most interesting problems in basic fullerene research. We have studied the formation mechanism of C60 fullerenes using first principles calculation and molecular dynamics simulations. We have derived a force field (MSX FF) that is suitable to describe both the sp1 hybrid and sp2 hybrid carbons. Combining DFT and MD with MSX FF we found the relative thermal stability of various neutral isomers at each cluster size n and predicted the relative abundancy of these neutral species for thermal equilibrium. We identified a complete path to form a C60 fullerene from atomic carbons and calculated its energetics. Our approach is fully applicable to other possible reaction paths and other fullerenes.
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