(
)
308
C. Buschhaus et al.rPhysics Letters A 256 1999 307–311
rather useful for the distinction of different carbon-
hydrogen centres.
tion of the unpaired spins with the remaining protons
in the pyrocarbon was characterised by Overhauser
w x
In this letter, we support the potentiality of mag-
netic measurements for the characterisation of the
pyrocarbon preparation process via CVD in hot wall
reactors. It was shown before that the combination of
measurements of electronic transport, thermal and
magnetic properties presents a specially reliable ba-
sis for the characterisation of different modifications
shift analysis 5 .
3. Discussion of the experimental results
w
x
According to the current understanding 1,2 , the
pyrocarbon formed under the experimental condi-
tions described above ought to approach a graphite-
like carbon modification with delocalised conduc-
tion electrons, unknown concentration of localised
w x
of carbon 4 . In the current investigation, pyrocar-
Ž
.
Ž
bon is deposited starting with methane on alumina
ceramic substrates and analysed with static and reso-
nant magnetic methods as free-standing film after
peeling off from the substrate.
.
Ž
.
Ž
.
defect spins e.g. at dangling bonds and a non-
negligible concentration of remaining protons due to
imperfect dehydration in the sequence methane —
heavier hydrocarbon — pyrocarbon. Isolated protons
may originate from CH groups at sp2 as well as sp3
carbon positions, proton pairs at CH2 groups with a
sp3 carbon configuration. These entities can be dis-
tinguished by static and resonant magnetic measure-
2. Experimental details
The pyrocarbon samples were prepared by chemi-
cal vapour deposition on alumina ceramic substrates
of 25 mm length, 20 mm width and 1 mm thickness.
A tubular reactor was used consisting of an alumina
ceramic reactor tube surrounding the conical inlet
nozzle and outlet fitting made of pyrophillite and the
central alumina ceramic tube forming the deposition
w
x
ments 6–8 .
3.1. Static magnetic susceptibility
The variation of the static magnetic susceptibility
of the non-oriented pyrocarbon sample with tempera-
ture measured in an external field of 30 kG flux
density is shown in Fig. 1. The solid line fit with a
temperature independent contribution and a Curie–
Weiss law
w
x
space and supporting the alumina substrate 1,2 . For
the sample preparation, an argon gas plug-flow with
Ž
a partial pressure of 500 mbar of methane total
.
pressure 1013 mbar , a reaction temperature of
11008C, a residence time of the vapour in the reactor
of 0.32 s and a total deposition time of 6 h were
adopted. Due to the difference in thermal expansion,
the thick film at the rear end of the substrate cracked
off during cool-down and could easily be peeled off.
The magnetic properties could thus be characterised
for such pyrocarbon films of several tens of microns
thickness free of substrate. Due to the growth pro-
cess, the pyrocarbon flakes were non-symmetrical
x sx qC r TyQ
1
Ž
.
Ž .
g
0
g
gives xo s1.3=10y6 emurg, Cg s0.6=10y4
emu Krg and Qsy3 K. Converted into approxi-
Ž
mate molar units i.e. with Mm f12 grmol C, ne-
.
glecting the hydrogen content , the Curie part of the
magnetic susceptibility — Cm f7.4=10y4 emu
Krmol C — indicates a concentration of 1.9=10y3
unpaired electron spins Ss1r2 per carbon atom, a
Ž
.
Ž
.
and had glossy lower and frosted upper surface.
Static magnetic susceptibility was measured at 30
kG flux density with a Quantum Design MPMS
SQUID magnetometer with the sample surrounded
during measurements by a low-pressure helium at-
mosphere.
w x
concentration that is not unusual for pyrocarbons 4 .
In the lower part of Fig. 1, the quantity xT is
plotted, that shows deviations from a pure Curie law
more clearly. The small deviation from the straight
line at low temperature and the small negative
Curie–Weiss temperature Qsy3 K of the fit to Eq.
Ž
.
X-band electron spin resonance ESR spectra at
9.5 GHz were recorded with a Bruker ESP 300 E
spectrometer equipped with an Oxford Instruments
variable temperature gas-flow cryostat. The interac-
Ž .
1 indicate weak antiferromagnetic interaction of the
localised spins, at least for part of them. The antifer-
romagnetic interaction is not sufficient, however, to