A transmission electron microscope study of individual soot grains forming fluffy carbon particles produced using the arc-discharge technique revealed close-packed arrangements of single-wall ring structures with average diameters of 0.7, 1.1, 3.0, 5.5 and 8.2 nanometers. These structures were hypothesized to be C60 and giant, C540, C960 and C1500, fullerenes that could form by coalescence during condensation and soot agglomeration although in situ solid-state growth cannot be excluded. Mass spectroscopy and HPLC chromatography of the samples confirmed the presence of C60 fullerene in all samples giving confidence to the giant fullerene growth scenario. Our results suggest that fullerenes could be common in soot grains produced by this technique as well as being an important carbon phase in C-rich accretion disks around young stellar objects and among the dust in the interstellar medium.
C60 and giant fullerenes in soot condensed in vapors with variable C/H2 ratio
ROTUNDI, Alessandra;
2004-01-01
Abstract
A transmission electron microscope study of individual soot grains forming fluffy carbon particles produced using the arc-discharge technique revealed close-packed arrangements of single-wall ring structures with average diameters of 0.7, 1.1, 3.0, 5.5 and 8.2 nanometers. These structures were hypothesized to be C60 and giant, C540, C960 and C1500, fullerenes that could form by coalescence during condensation and soot agglomeration although in situ solid-state growth cannot be excluded. Mass spectroscopy and HPLC chromatography of the samples confirmed the presence of C60 fullerene in all samples giving confidence to the giant fullerene growth scenario. Our results suggest that fullerenes could be common in soot grains produced by this technique as well as being an important carbon phase in C-rich accretion disks around young stellar objects and among the dust in the interstellar medium.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
