Serge A Krasnokutski1, Martin Kuhn2, Alexander Kaiser2, Andreas Mauracher2, Michael Renzler2, Diethard K Bohme3, Paul Scheier2. 1. Laboratory Astrophysics Group of the Max Planck Institute for Astronomy at the Friedrich Schiller University Jena , Helmholtzweg 3, D-07743 Jena, Germany. 2. Institut für Ionenphysik und Angewandte Physik, Universität Innsbruck , Technikerstr. 25, A-6020 Innsbruck, Austria. 3. Department of Chemistry, York University , 4700 Keele Street, Toronto M3J 1P3, Ontario, Canada.
Abstract
We report the observation of sequential encounters of fullerenes with C atoms in an extremely cold environment. Experiments were performed with helium droplets at 0.37 K doped with C60 molecules and C atoms derived from a novel, pure source of C atoms. Very high-resolution mass spectra revealed the formation of carbenes of the type C60(C:)n with n up to 6. Bridge-type bonding of the C adatoms to form the known dumbbell C60═C═C60 also was observed. Density functional theory calculations were performed that elucidated the carbene character of the C60(C:)n species and their structures. Mass spectra taken in the presence of water impurities and in separate experiments with added H2 also revealed the formation of the adducts C60C(n)(H2O)n and C60C(n)(H2)n probably by H-OH and H-H bond insertion, respectively, and nonreactivity for the dumbell. So C adatoms that form carbenes C60(C:)n can endow pristine C60 with a higher chemical reactivity.
We report the observation of sequential encounters of fullerenes with C atoms in an extremely cold environment. Experiments were performed with helium droplets at 0.37 K doped with C60 molecules and C atoms derived from a novel, pure source of C atoms. Very high-resolution mass spectra revealed the formation of carbenes of the type C60(C:)n with n up to 6. Bridge-type bonding of the C adatoms to form the known dumbbell C60═C═C60 also was observed. Density functional theory calculations were performed that elucidated the carbene character of the C60(C:)n species and their structures. Mass spectra taken in the presence of water impurities and in separate experiments with added H2 also revealed the formation of the adducts C60C(n)(H2O)n and C60C(n)(H2)n probably by H-OH and H-H bond insertion, respectively, and nonreactivity for the dumbell. So C adatoms that form carbenes C60(C:)n can endow pristine C60 with a higher chemical reactivity.
Since the
discovery of fullerene
in vaporized graphite and its assignment by Kroto et al. and confirmation
by Krätschmer et al.,[1,2] the growth mechanisms
of fullerene formation under energetic conditions have been a matter
of debate.[3−6] Simultaneously, several routes to add functional parts to fullerenes
have been highly successful, including cyclopropanation, Diels–Alder
reactions, and carbene additions.[7−9] Derivatized fullerenes
have promising applications in material and life sciences.[10−12] They are used as electron acceptor molecules in solution-processed
organic photovoltaic cells,[13] they are
considered for biological and medical applications,[14,15] for DNA manipulation,[16] and for biosensors,[17] and they have been successfully deposited on
surfaces as novel self-assembled monolayers.[18] The possibility of activating reactive fullerenes with C atoms to
form carbenes that can promote subsequent fullerene derivatization
has driven us to investigate these species more closely. We performed
laboratory experiments designed to explore encounters of fullerenes
with C atoms derived from a clean source of C atoms.[19] Such encounters may also occur in natural environments
such as interstellar space where C60 and C60+ have been detected.[20,21] Quite recent
experiments under energetic conditions with laser-ablated carbon vapor
and C60 under a flow of helium suggest that the carbon
vapor can promote C exchange, C60 isomerization, and C
atom incorporation, leading to fullerene closed network growth under
these conditions.[6,22] Also, under the hot conditions
in fullerene plasma experiments, Shvartsburg et al. proposed the existence
of ball-and-chain type fullerene dimers connected with one or more
C atoms.[23] C additions to C60 were also predicted to catalyze Stone–Wales transformations.[24]There has been a recent breakthrough in
pure C atom production.
Low-energy carbon atoms now can be produced with a purity >99%
from
a thin-walled, sealed tantalum tube containing carbon.[19] We have adopted this source to investigate the
reactivity of C60 toward C atoms in very low-temperature
He droplets and modified our apparatus that allows C60 molecules
to be added into He droplets (ca. 106 He atoms and five
C60 molecules on average per droplet) where they can aggregate
and be cooled to the droplet temperature of 0.37 K.[25] Carbon atoms are then added and allowed to react with the
C60 aggregates before the droplets are exposed to ionizing
or attaching electrons that permit reactants and products to be analyzed
with a mass spectrometer. While low-energy (<22 eV) electrons can
attach directly, higher energy electrons (>22 eV) first generate
either
He+ or He*– that then ionizes neutrals
inside the droplet.[26−29] To vary the C input into the droplet, the electric power used to
heat the tantalum tube was varied from ca. 60 to 162 W.Mass
spectra recorded for adduct formation with up to six carbon
atoms to C60 are shown in Figure . The two stable isotopes of carbon, 12C (98.93%) and 13C (1.07%), lead to a characteristic
series of mass peaks when combined with molecules or clusters (binomial
statistics). The peak pattern of the mass spectrum of the negatively
charged ions from m/z = 720 to 725
perfectly matches the calculated isotopic pattern of C60, whereas the subsequent groups of mass peaks assigned to C6013C– (n = 1 to 6) exhibit enhanced intensity for the fifth isotopologue 12C5513C, which can be attributed to water, replacing one 13C
(12C6013CH2O).
Figure 1
Mass spectra recorded for C60C+ (bottom) and C60C– ions (top) for He droplets (nozzle
temperature
9.5 and 9.7 K, respectively) containing C60 and 13C atoms. The ionizing energies are 70 and 22 eV, the C60 oven temperatures were 292 and 288 °C, and the power settings
for the 13C source were 158 and 162 W, respectively. Note
the presence of water impurities. (See the text.) The inset shows
enlarged the range of the dication (C60)2C2+. The thin line shows the corresponding monocation plotted
with the mass scale divided by two.
Mass spectra recorded for C60C+ (bottom) and C60C– ions (top) for He droplets (nozzle
temperature
9.5 and 9.7 K, respectively) containing C60 and 13C atoms. The ionizing energies are 70 and 22 eV, the C60 oven temperatures were 292 and 288 °C, and the power settings
for the 13C source were 158 and 162 W, respectively. Note
the presence of water impurities. (See the text.) The inset shows
enlarged the range of the dication (C60)2C2+. The thin line shows the corresponding monocation plotted
with the mass scale divided by two.Remarkably, the observed mass distribution is quite similar
for
positive and negative ions despite the substantial differences in
the mode of ionization. Positively charged ions are predominantly
formed via charge transfer from an initially formed He+ ion, which approaches the C60C via resonant hole-hopping,[30] whereas
the dominant process for anion formation at 22 eV is due to He*–, which is resonantly formed at this electron energy
and attracted by the polarizable C60C.[31] The electronic energy of He+ and He*– is almost the same, and thus similarity
in the spectra is expected if the C atoms attach to C60 in neutral reactions first and the products are subsequently ionized.
The occurrence of dissociative ionization accompanied by loss of one
or more C atoms from higher members of the series could not be excluded.Similarity in the positive and negative ion spectra is expected
if the C attaches to C60 in neutral reactions first, and
the products are subsequently ionized. The structures of the C60(C) molecules that are formed
are not known from these experiments; sequential attachment of C atoms
can proceed either only on the surface of the C60 by bridge
addition (Figure a–c,g–i)
or in the formation of a C chain (Figure d,f) extending away from the surface, as
in C60=C=C=C=C=C=C:,
or in an intermediate fashion. Fullerene growth (Figure e) by C2 insertion
can be largely excluded because it is unlikely that two carbon atoms
adsorb next to each other at the same hexagonal or pentagonal face.
The adatoms should be immobile once they are adsorbed at these low
temperatures.
Figure 2
(a) Lone pair orbital at the C-adatom in singlet C61 [6,5] from a natural bond orbital analysis.[34] Structures computed with DFT calculations for C62 (b–e),
C63 (f), C64 (g), and C66 (h,i).
(a) Lone pair orbital at the C-adatom in singlet C61 [6,5] from a natural bond orbital analysis.[34] Structures computed with DFT calculations for C62 (b–e),
C63 (f), C64 (g), and C66 (h,i).Computations indicate that a single
carbon adatom chemically binds
to the C60 cage at both distinguishable bond positions,
that is, between two hexagonal faces [6,6] with 3.09 eV or one hexagonal
and a pentagonal face [6,5] with 2.83 eV.[32] Later density functional theory (DFT) calculations identified the
[6,5] bridge as the most stable favored by 0.3 eV.[33] Our own DFT calculations with results summarized in Table
1S in the Supporting Information agree
with this latter stability order; we found that the [6,5] bond is
slightly preferred to the [6,6] bond with a bond energy De (dissociation energy of the carbon adatom) of 2.82 eV
on the [6,5] bond. This compares with 3.52 eV for the cation and 3.39
eV for the anion. C60C also was seen to have carbene properties
from a natural bond orbital analysis.[34] The resulting doubly occupied lone-pair orbital of the 61st carbon
atom in singlet C61 is shown in Figure a. Further calculations provided an ionization
energy of 6.37 eV for C61, significantly smaller than 7.08
eV for C60, and an electron affinity of 2.43 eV, larger
than 2.25 eV for C60, and a fairly large dipole moment
of 1.2765 D (with μ = 1.1855 D,
μ = 0.0000 D, and μ = 0.4735 D).In the case of two carbon adatoms,
the reference structure is shown
in Figure b with two
[6,6] C adatoms that are situated normal to each other with respect
to the fullerene center. The adatoms can also adsorb very close to
each other on neighboring bonds of a single carbon hexagon (Figure c); this structure
is only 0.013 eV less stable than the reference structure, an amount
that is not significant for DFT. We also considered other structures.
A high-energy gain of 3.97 eV compared with the structure shown in Figure b can be reached
by adsorbing the two carbon atoms in a bent chain on a [6,6] position,
as shown in Figure d. Adsorption of two carbon atoms at opposite bonds of a pentagon
face leads without barrier to a very stable (−5.3 eV) C62 cage structure with two heptagons and a tetragon (almost
square, Figure e).
In this noncarbene cage all carbon atoms are bound to three neighbors,
and lone pairs are absent in the natural bond orbital analysis.For C63 (C64) we find that adsorption of
a C–C–C (C–C–C–C) chain on a [6,6]
position is energetically favorable by −7.13 eV (−10.83
eV) compared with distributed single adatoms. The C–C–C
structure for C63 is shown in Figure f and that of the distributed single adatom
structure for C64 is shown in Figure g. The perfectly symmetric structure for
C66 with six single carbon adatoms at [6,6] positions (Figure h) is energetically
unfavorable by only 0.038 eV compared with 6 C adatoms at [6,5] positions,
as shown in Figure i. We did not calculate chain structures for more than four adatoms.
Adding an additional C atom to the perfectly symmetric C66 gives C67. The dissociation energies for distributed
adatoms from C61 to C66 lie in a range of 2.49
to 2.82 eV for one to six carbons. For seven adatoms the dissociation
energy decreases to 1.94 eV. In the latter case the C60 cage distorts more. The typical bond length of the [6,6] bond, where
C is adsorbed, is 1.582 Å for C66. For two of the
seven C adatoms in C67, this bond length is stretched to
1.618 Å.In summary, the computations predict the existence
of a variety
of different stable isomers for which fullerene cage growth[6,22] is energetically favorable compared with C–C–···
chain attachment, which is, in turn, favorable to the well-separated
addition of up to at least seven single C atoms. The well-separated
addition is proposed to occur in our experiments in a cold environment
due to rapid cooling accompanied by trapping in local minima on the
potential energy surface,[35] whereas cage
growth is likely favored at higher temperatures as in the experiments
of Dunk et al.[6,22] The carbene character of bridge-type
C60(C:) is clearly manifested
by the natural bond orbital analysis that is displayed in Figure a for C60(C:)1.Carbene character can be inferred for all
experimentally observed
C adducts C60(C) from the
observed water impurity adduct C60C(H2O)± ion peaks in Figure . According to the presence of these peaks, C60(C) molecules with n > 0
pick
up H2O, as would be expected from a carbene reaction, presumably
by H–OH bond insertion, while C60 itself adds H2O only by physisorption. Furthermore, the results of our separate
experiments with added H2 dopant (see Figure and Figures 1S and 3S in the Supporting Information) indicate H2 additions for each C60(C) with n = 1,2,3,4,5, presumably by H–H bond
insertion. These results with H2O and H2 strongly
indicate sequential surface addition of at least
the first five carbon atoms to form carbenes of the type C60(C:) with n = 1–5
instead of energetically favorable C chains such as C60=C=C=C=C:, for which always only one
H2O or H2 would add chemically (H2 at T = 0.37 K does not add chemically to C60 because of a large barrier predicted to be 1.69 eV).[36] This result shows that C-atom additions can
transform a chemically inert (against reaction with H2 and
H2O) fullerene C60 into chemically reactive
carbenes C60(C:). Carbenes
are known from terrestrial chemistry to be among the most versatile
and synthetically useful reactive intermediates. Carbene additions
to fullerenes have already attracted considerable attention.[8] Carbenes should also play a similar role in interstellar
chemistry.[37] Our experiments demonstrate
the reactivity of C60(C:) toward
H2 and H2O. We expect similar reactivities toward
many other molecules as well as other carbenes such as :CO, :CS, :C:, :CO, and
:CNH, for example.[37]
Figure 3
Mass spectra recorded
for 12C6013CHn+ ions for
droplets containing C60, 13C, and H2. The ionizing energy is 70 eV, the C60 oven temperature
is 292 °C, the power setting for the 13C source was
162 W. The ambient pressure of H2 was 0.5 mPa.
Mass spectra recorded
for 12C6013CHn+ ions for
droplets containing C60, 13C, and H2. The ionizing energy is 70 eV, the C60 oven temperature
is 292 °C, the power setting for the 13C source was
162 W. The ambient pressure of H2 was 0.5 mPa.Our other recorded mass spectra show evidence of
the presence of
C adduct ions for clusters of fullerenes of the type (C60)(C)± with n = 1 to 9 and m = 1–5 including the dumbbell. Excerpts are shown in Figure for (C60)2(C)± with m = 0–3. The positive and negative ion spectra both
show a remarkable predominance of ionized (C60)2C, suggesting the occurrence of neutral chemistry before ionization
and a special stability for neutral (C60)2C,
presumably the dumbbell C60=C=C60. The concomitant observation of the dication (C60)2C2+ (see insert in Figure ) as well as experiments with additional
H2 dopant completely support this assignment. The dication
appears to be stable against Coulomb explosion; presumably the two
charges are located apart on the two fullerenes. H2 is
seen in Figure to
add to (C60)2C2, in which the second
C atom is attached to one of the fullerenes and so is available to
insert into the H–H bond but not (C60)2C, in which the C atom is not accessible in the dumbbell configuration.
Figure 4
Upper
part: Mass spectra recorded for C60C+/(C60)2C+ ions (left) and C60C–/(C60)2C– ions (right)
for He droplets (nozzle temperature 9.5 and 9.6 K, respectively) containing
C60 and 13C atoms. The ionizing energies are
90 and 22 eV, the C60 oven temperatures were 308 and 300
°C, and the power settings for the 13C source were
141 and 150 W, respectively. Note the presence of water impurities
(see text). Lower part: Mass spectra recorded for (C60)213CH+ ions for droplets containing C60, 13C, and H2. The ionizing energy is 70 eV, the C60 oven temperatures is 292 °C, and the power setting
for the 13C source was 162 W. The ambient pressure of H2 was 0.5 mPa.
Upper
part: Mass spectra recorded for C60C+/(C60)2C+ ions (left) and C60C–/(C60)2C– ions (right)
for He droplets (nozzle temperature 9.5 and 9.6 K, respectively) containing
C60 and 13C atoms. The ionizing energies are
90 and 22 eV, the C60 oven temperatures were 308 and 300
°C, and the power settings for the 13C source were
141 and 150 W, respectively. Note the presence of water impurities
(see text). Lower part: Mass spectra recorded for (C60)213CH+ ions for droplets containing C60, 13C, and H2. The ionizing energy is 70 eV, the C60 oven temperatures is 292 °C, and the power setting
for the 13C source was 162 W. The ambient pressure of H2 was 0.5 mPa.The stability of the bridged dumbbell structure C60=C=C60 is well known from terrestrial chemistry.[38] C121 has been previously detected
in the laboratory
by mass spectrometry[39] of the products
obtained in the synthesis of C61Br2 from C60 and C6H5HgCBr3 and has
been isolated using thermolysis of a mixture of C60 and
C60CBr2 or the neutron irradiation of pure C60.[40] Photochemical and photophysical
properties of the three bridged isomers [6,6]–[6,6], [5,6]–[6,6],
and [5,6]–[5,6] also have been reported.[41,42]Under energetic conditions C and C2 addition to
fullerenes
leads to closed network growth as demonstrated by Kroto et al.,[6,22] whereas our observed surface C additions at low temperature enhance
the chemical activity of the surface of C60 by carbene
formation. The latter may pave the way toward a generation of a new
class of fullerene derivatives. Reactive C60 carbene species
may also be formed in interstellar and circumstellar environments
containing C and C60, where they could add H2 and H2O, as well as C60, to form derivatized
fullerene molecules such as C60(CH(H)), C60(CH(OH)), C60(C=CO), and even C60(C=C60).
Experimental
Section
He droplets were formed by expanding helium (Messer
purity 99.9999%)
from a stagnation pressure of 2.4 MPa through a 5 μm nozzle,
cooled by a closed-cycle refrigerator (Sumitomo Heavy Industries LTD,
model RDK-415D) to ∼9.5 K, into vacuum. The average size of
the He droplets is ∼106 atoms.[43] The resulting supersonic beam was skimmed by a 0.8 mm conical
skimmer located 1 cm downstream from the nozzle and flew through two
10 cm long, differentially pumped pick-up regions. Small amounts of
C60 (MER, purity 99.9%) were vaporized at an oven temperature
between 292 and 308 °C and picked up by the He droplets with
almost unity efficiency upon collisions. In the second differentially
pumped pickup chamber atomic (purity >99%) vapor of 13C
emitted from a heated sealed tantalum tube containing carbon is picked
up by the He droplets.[19] H2 (Messer,
purity 99.999%) was introduced via an electronically controlled leak
valve into the first pickup chamber. Water was present in the machine
as a trace impurity from the residual gas. The doped helium droplets
were ionized by collisions with electrons at energies ranging from
0 to 100 eV. The ions were accelerated to 40 eV into the extraction
region of a commercial orthogonal time-of-flight mass spectrometer
equipped with a reflectron (Tofwerk AG, model HTOF). For anions the
mass resolution was m/Δm =
2500 and for cations 3500. The base pressure in the mass spectrometer
was 10–5 Pa. The ions were detected by a microchannel
plate and recorded via a time to digital converter. Additional experimental
details have been described elsewhere.[44] Special home-built software was utilized to deduce ion intensities
from the mass spectra, taking into account all possible isotopologues,
as shown in Figure 2S in the Supporting Information.[45]Energetics and geometries of
neutral C60 with carbon
adatoms were calculated by means of DFT. All structures were fully
optimized to account for deformations of the fullerene due to the
presence of the carbon adatoms. We used the B3LYP[46,47] hybrid density functional and a standard 6-31g(d)[48] basis set as implemented in the Gaussian 09 program.[49] Energies were corrected for zero-point vibrations,
and all reported structures are true local minima. The accuracy of
isomerization energies and heats of formation of B3LYP with the 6-31g(d)
basis set was estimated with 0.13 eV for a large set of neutral, closed-shell
organic compounds containing C, H, N, and O.[50]
Authors: Lukas An der Lan; Peter Bartl; Christian Leidlmair; Harald Schöbel; Roland Jochum; Stephan Denifl; Tilmann D Märk; Andrew M Ellis; Paul Scheier Journal: J Chem Phys Date: 2011-07-28 Impact factor: 3.488
Authors: Paul W Dunk; Nathan K Kaiser; Christopher L Hendrickson; John P Quinn; Christopher P Ewels; Yusuke Nakanishi; Yuki Sasaki; Hisanori Shinohara; Alan G Marshall; Harold W Kroto Journal: Nat Commun Date: 2012-05-22 Impact factor: 14.919
Authors: Stefan Ralser; Johannes Postler; Martina Harnisch; Andrew M Ellis; Paul Scheier Journal: Int J Mass Spectrom Date: 2015-03-15 Impact factor: 1.986
Authors: Andreas Mauracher; Matthias Daxner; Johannes Postler; Stefan E Huber; Stephan Denifl; Paul Scheier; J Peter Toennies Journal: J Phys Chem Lett Date: 2014-06-20 Impact factor: 6.475