Laboratory studies of ion/molecule reactions of fullerenes: Chemical derivatization of fullerenes within dense interstellar clouds and circumstellar shells
S. Petrie et Dk. Bohme, Laboratory studies of ion/molecule reactions of fullerenes: Chemical derivatization of fullerenes within dense interstellar clouds and circumstellar shells, ASTROPHYS J, 540(2), 2000, pp. 869-885
We discuss recent experimental results for ion/molecule reactions of ionize
d and multiply-ionized fullerenes, and of derivatized fullerene ions, with
molecules relevant to the chemistry of interstellar clouds and circumstella
r envelopes These reactions were studied using a selected-ion how tube (SIF
T) at 294 +/- 2 K in helium at a pressure of 0.35 +/- 0.01 torr. The presen
t study supplements an earlier discussion on aspects of interstellar fuller
ene ion chemistry explored by the same technique. Several implications are
apparent for the chemical processing of fullerenes in various astrophysical
environments. Triply charged fullerene ions, such as C-60(3+), may be form
ed under conditions prevailing within dense IS clouds, but their abundance
will be very low owing to the large number of loss processes identified for
such species. Derivatization of fullerene ions under interstellar or circu
mstellar conditions is less probable for larger fullerenes than for fullere
nes smaller than C-60. Hydrogenation may severely impede the efficiency of
fullerene ion association with polar molecules and small unsaturated molecu
les, but should not substantially affect the efficiency of addition of radi
cals or PAHs under these conditions.
We discuss prospects for neutralization of ionized fullerene adducts. Four
classes of adduct ions are described, differing in their structure and expe
cted neutralization tendencies. Adducts of fullerene ions with interstellar
isonitriles, with radicals, and with linear polycylic aromatic hydrocarbon
s (PAHs; class 1) are most likely to form derivatized fullerenes on neutral
ization, while fullerene ion adducts of nitriles, most hydrocarbons (class
3), and nonlinear PAHs (class 4) are most likely to yield the bare fulleren
e cage upon neutralization. Adducts of ammonia (class 2) appear to have an
intermediate probability of surviving neutralization with the functionalizi
ng group(s) intact.