Z.L. Wang, J.S. YinrChemical Physics Letters 289 (1998) 189–192
191
that the local Ž001. graphite plane is nearly perpen-
dicular to the electron beam. The continuous Ž101.
and Ž112. rings mean the random twist among Ž001.
graphitic layers forming the shell. When the electron
beam is positioned at the edge of the calabash ŽFig.
EDS spectrum acquired from the edge of a solid
carbon sphere ŽFig. 3c. shows a negligible oxygen
peak, indicating that the oxygen adsorbed on the
carbon surface, if any, is vanishingly small. Quanti-
tative analysis of Fig. 3a gives the atom ratio of
wn rn x sŽ2.3"0.3.%, where the oxygen signal
2
c., the pattern shows an arc-shape of the Ž002. and
O
C Ža.
Ž004. reflections due to the curvature of the graphitic
is contributed by the adsorbed oxygen and the oxy-
gen gas enclosed inside the shell. In the case of Fig.
3b, wn rn x sŽ0.5"0.3.%, and the oxygen sig-
layers, thus, the Ž001. plane is nearly parallel to the
electron beam, in agreement with the result provided
by the TEM image. The elliptical shape of the Ž101.
O
C Žb.
nal is dominated by the adsorbed oxygen on the
shell. With consideration the large size of the cal-
abash in comparison to the beam size, the volume
density of oxygen rO enclosed inside the shell is
determined by
reflection is due to the spherical shape of the graphitic
layers, and it indicates that the size of the graphitic
layer is large w19x. This elliptical shape is a distinct
difference from the diffraction pattern recorded from
a solid carbon sphere composed of small-size
graphitic flakes w15–18x.
ro yri
ri
rO f
Ä
wn rn x y2wn rn xŽb.4r ,
O
C
O
C
C
1
Ž .
Ža.
From the TEM images presented above it can be
concluded that the carbon calabashes are either hol-
low or containing a carbon core. It is our interest to
find the type of gas enclosed inside the calabashes.
To probe this phenomenon from a single carbon
calabash, EDS in TEM was employed. The electron
beam was focused to a size of 30 nm, so that the
chemical composition of the carbon calabash, as
shown in the inset of Fig. 3, can be detected near its
center and at its edge. In reference to the carbon
K line, the oxygen K line in the EDS spectrum
acquired from the center of the calabash shell ŽFig.
where r and r are the outer and inner radii of the
o
i
shell, respectively, and rC is the atom volume den-
sity of graphite. From the kinetics of gases, the
partial pressure of oxygen is given by
rO
PO s
RT ,
2
Ž .
NA
where NA is the Avogadro’s number, R the gas
constant and T temperature. For Ts300 K and Žr
o
5
y r .rr s 0.04, Eq. Ž2. yields P f 2.4 =10
i
i
O
2
Nrm . This means that the oxygen partial pressure
inside the calabash is ;2.4 atmospheric pressure.
This is a reasonable number with consideration of
our experimental condition.
3
a. is apparently stronger than that in the spectrum
acquired from the edge of the shell ŽFig. 3b.. The
The gases trapped inside the hollow carbon cal-
abashes can be oxygen, hydrogen andror CH . If
4
the trapped oxygen were in solid state and were
distributed uniformly on the surface of the inner
shell, there would be no difference between the EDS
spectra acquired when the electron probe was posi-
tioned at the center and at the edge of the shell. The
oxygen could be provided by the MnOx catalysis
during the carbonization process.
From the literature, a curling graphitic carbon
particle is believed to be nucleated from a pentago-
nal atom ring, and its growth gives a quasi-icosa-
Fig. 3. Energy-dispersive X-ray spectra acquired from Ža. the
center of a carbon calabash, Žb. the edge of the calabash, and Žc.
the edge of a solid carbon sphere. The Cu L line came from the
copper grid used in TEM analysis. The relative intensity of the Cu
L line with respect to that of the carbon K line depends on the
specimen thickness, but the relative magnitude of O K line to C
K line is the intrinsic property of the local region.
hedral spiral shell carbon particle 20,21 . A pentago-
nal carbon ring produces an inward surface with
positive curvature, resulting in spiral growth. This
has been proposed as the nucleation of fullerenes and
solid carbon spheres w15–18,20,21x. The structure of
w
x