Laboratory studies of ion/molecule reactions of fullerenes: Chemical derivatization of fullerenes within dense interstellar clouds and circumstellar shells

Citation
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
Citations number
123
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
540
Issue
2
Year of publication
2000
Part
1
Pages
869 - 885
Database
ISI
SICI code
0004-637X(20000910)540:2<869:LSOIRO>2.0.ZU;2-W
Abstract
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.