Appl. Phys. Lett., Vol. 78, No. 8, 19 February 2001
Tan et al.
1085
The variation in the amorphous silicon tunnel barrier
height may be explained by considering the dopant distribu-
tion in the nc-Si film. A nc-Si grain of 4 nm diameter con-
tains on average thirty phosphorous atoms while a 0.5 nm
thick amorphous silicon grain boundary contains on average
only six phosphorous atoms. This implies that the grain
boundaries would be strongly influenced by any fluctuation
in the doping concentration, leading to a variation in the
energy difference between the conduction band edge and the
Fermi level in the amorphous silicon, and a variation in the
depletion width at the crystalline silicon/amorphous silicon
interface. We note that if the tunnel barrier on average is 40
meV high and 0.5 nm wide, the tunnel resistance is ϳ10 k⍀,
which is less than the quantum resistance R ϭ25.8 k⍀ and
K
1
1
Coulomb blockade effects are not possible. However, in
our measurements there must be a wider than average grain
boundary because of statistical fluctuations in the grain
boundary width together with additional depletion regions on
either side. This would create a wider tunnel barrier with a
higher tunnel resistance, for example if the barrier is 40 meV
high and 2 nm wide, the tunnel resistance is ϳ10RK and
Coulomb blockade effects would occur.
We have also fabricated up to 60 nm wide devices which
exhibit a maximum tunnel barrier height from 16–22 meV.
In these devices a larger number of percolation paths may
exist for electron transport and a lower tunnel barrier height
is more likely observed. Even in the point contact device of
Fig. 4, the maximum barrier height of 40 meV is relatively
low for electronic confinement at higher temperatures closer
FIG. 4. ͑a͒ Arrhenius plot of Vds biased at 50 mV ͑circles͒ and at zero
biased ͑triangles͒. T1 indicates the transition temperature, ϳ60 K, and EAl is
the maximum gradient obtained from the region for 60 KϽtemperature
Ͻ300 K, as indicated by the first solid line. The second and third solid line
to room temperature. At temperatures ϾT , single-electron
1
Ϫ1
effects disappear and there is a transition to percolation con-
duction.
shows the T dependence. ͑b͒ For 60 KϽtemperatureϽ300 K, the results
Ϫ1/4
follow a T
dependence as shown by the solid lines.
In conclusion, we have observed single-electron effects
in nc-Si point contacts up to a temperature of 60 K. We have
shown that the charging islands are nc-Si grains as small as
ϳ4 nm, isolated by amorphous silicon regions ϳ0.5 nm
thick. Electron transport is attributed to a thermally assisted
single-electron tunneling process at low temperature and per-
colation conduction at high temperature. Our work is funded
by the Japan Science and Technology Agency CREST pro-
gram.
ϭ50 mV, the device operates outside the Coulomb gap.
From 6 K to a transition temperature T ϳ60 K, log() fol-
1
Ϫ1
lows a T
T
dependence and above T , log() follows a
1
Ϫ1/4
Ϫ1/4
dependence. In the region of the T
dependence, the
conduction mechanism is likely to be dominated by percola-
tion conduction through a distribution of potential barrier
1
2
heights with various activation energies. The maximum
Ϫ1/4
gradient obtained from the region of T
dependence cor-
responds to an activation energy EA1ϳ40 meV, which can
1
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Ϫ1
silicon tunnel barrier in the nc-Si. The region of T depen-
2
dence corresponds to a smaller activation energy EA2
ϳ3 meV. This value is too low for electronic confinement
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1
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similar to that measured at V ϭ50 mV. This is because the
ds
Coulomb gap in the device disappears at ϳT and the zero
1
9
bias conductivity is similar to the conductivity at V
10
ds
Ϫ1
ϭ50 mV. Below T , there again exists a T
dependence.
1
11
However, the activation energy EA3ϳ10 meV is larger. This
energy is close to the Coulomb charging energy ϳ15 meV
obtained for the dominant island from the gate oscillations of
12
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Fig. 3͑b͒.
͑1973͒.
1
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