A series of cationic
molecular fragments (C
n
+, n = 11, 12, 15, 16,
18, and 21), produced by electron-impact ionization
of C60 in the gas phase, were each mass-selected and accumulated
in cryogenic Ne matrices. Optical absorption measurements in the UV–vis
and IR spectral ranges reveal linear carbon chain structures. In particular,
we have observed the known electronic transitions of linear C11, C15, and C21. The NIR transitions
of linear C15
–, C16
–, and C18
– have also been detected, indicating that soft-landing of the corresponding
cations can also involve charge-changing. Newly observed electronic
absorptions at 410.3 and 429.9 nm have been assigned to linear C18 absorptions at 438.2, 443.5, 422.3, and 433.7 nm, to linear
C15
+, and absorption
at 395.5 nm, to linear C16. Increasing deposition energy
leads to fragmentation upon impact. This is indicated by absorptions
of C10 (313, 316.3 nm), when depositing C
n
+ (n = 11, 15, 16) as well as C12 (332 nm) or C14 (347.4, 356.6 nm), when depositing C15
+ or C16
+, respectively. These were previously assigned
to cyclic isomers. We reassign them to linear isomers here on the
basis of plausibility arguments. The observations have been supported
by time-dependent density functional theory calculations for ring
and chain isomers of C
n
+/–/0, 10 ≤ n ≤ 20 up to the vacuum-UV range. The electronic absorptions
of carbon chains are at least 1 order of magnitude stronger than all
NIR electronic absorptions of C60
+, which have recently been attributed to several
of the diffuse interstellar bands. Considering that fullerene multifragmentation
yields long carbon chains that have very strong absorptions both in
the UV–vis and IR spectral regions, these systems appear to
be good candidates to be observed in regions of space containing fullerenes.