A. Jauhiainen et al., STEADY-STATE AND TRANSIENT CURRENT TRANSPORT IN UNDOPED POLYCRYSTALLINE DIAMOND FILMS, Journal of applied physics, 82(10), 1997, pp. 4966-4976
We have investigated steady-state and transient electrical properties
of undoped polycrystalline diamond thin films deposited using hot fila
ment chemical vapor deposition on (100)-oriented n-type and p-type sil
icon substrates. The capacitance-voltage characteristics are strongly
influenced by slow traps located close to the interface between the di
amond layer and the silicon substrate. When interpreting data one has
to consider that the traps are not in thermal equilibrium-during measu
rements. The steady-state current through the diamond him has the same
behavior for films deposited on both n-Si and p-Si. Its temperature a
nd held dependency can be interpreted in terms of Poole-Frenkel transp
ort involving ionized sites with overlapping potentials in the diamond
film. Electrically excited current transients decay with time accordi
ng to a power law. The kinetics depend only weakly on temperature. Fur
ther, the transients contain very long time scales and show much simil
arity to earlier reported optically excited ones. The temperature and
voltage dependency of the transient current magnitude are similar to t
he ones of the steady-state current for a nonzero field across the dia
mond layer during the transient. It is possible to qualitatively accou
nt for the steady-state and transient transport within the framework o
f the same basic model assuming that the traps involved in the transpo
rt have a certain spatial and energy distribution. From an application
point of view the leakage currents in the diamond film are of accepta
ble magnitude for many diamond based silicon-on-insulator applications
intended for operation at moderate temperatures and voltages. Finally
, the films also show promising behavior with respect to material reli
ability; from the electrical measurements no sign of degradation of th
e diamond films due to long term current stress can be seen. (C) 1997
American Institute of Physics.