Ultrathin Cu films with thicknesses d between similar to 10 and 40 nm were
thermally evaporated onto similar to 500-nm thick SiO2 on Si(100) substrate
s in an ultra high vacuum (UHV) chamber with a base pressure of 5 x 10(-10)
torr. The sheet resistance R (Omega/square), was measured in situ at diffe
rent film thicknesses by a collinear four-point probe. The infinite R at d
< 10 nm suggested that the film consisted of discontinuous islands at these
thicknesses. The R-value dropped rapidly by more than an order of magnitud
e when the thickness was increased from 10 to 15 nm, indicating the coalesc
ence of islands. Further increases in d resulted in the R value gradually l
eveling off at 0.65 +/- 0.01 <Omega>/square, corresponding to a resistivity
rho of 2.67 mu Omega cm at d similar to 41 nm. The rho -d data were fitted
by models that assume surface, interface and grain boundary scattering to
be dominant mechanisms for the thickness dependence on resistivity. Models
that do not include surface roughness do not fit our data in the sub-15-nm
thick Cu films regime. The surface roughness was measured by atomic force m
icroscopy (AFM). Our analysis shows that Namba's model that uses the measur
ed surface roughness provides the best description of the resistivity-thick
ness behavior in sub-40-nm thick Cu films. (C) 2001 Elsevier Science B.V. A
ll rights reserved.