Ka. Pacheco et al., GROWTH AND CHARACTERIZATION OF SILICON THIN-FILMS EMPLOYING SUPERSONIC JETS, Journal of vacuum science & technology. A. Vacuum, surfaces, and films, 15(4), 1997, pp. 2190-2195
Citations number
34
Categorie Soggetti
Physics, Applied","Materials Science, Coatings & Films
Supersonic jets of Si2H6 have been employed to grow single crystalline
silicon thin films on Si(100) and polysilicon surfaces at substrate t
emperatures of 500-650 degrees C. Films deposited on Si(100) employing
high and low kinetic energy jets are epitaxial as determined by refle
ction high energy electron diffraction. The uniformity and growth of f
ilms deposited on polysilicon by high energy similar to 2 eV (1% Si2H6
in hydrogen) and low energy similar to 0.09 eV (pure Si2H6) Si2H6 jet
s are compared to silicon growth employing ultrahigh vacuum chemical v
apor deposition (UHV-CVD). To ascertain the influence of high kinetic
energy on the growth of silicon from disilane, the reaction probabilit
y is estimated from growth measurements for all techniques and compare
d. The high energy jet is found to have a substantially higher reactio
n probability compared to the low energy jet and UHV-CVD indicating th
at the growth is enhanced by the high energy disilane. The disilane fl
ux distribution employing the high energy jet is sharply peaked along
the centerline causing a peaked growth profile across the 4 in. wafer.
The silicon growth profile obtained from the high energy jet broadens
slightly as the substrate temperature decreases. The higher flux at t
he centerline results in a higher hydrogen coverage compared to the wa
fer edge which affects the reaction probability in the two locations r
elative to one another. As the substrate temperature decreases, the gr
owth profile flattens since the lower hydrogen desorption rate, and re
sulting higher hydrogen coverage, reduces the disilane adsorption prob
ability at the centerline more than at the wafer edge. The growth dist
ribution from the high energy jet is found to become slightly less pea
ked when the carrier gas is changed from hydrogen to helium. (C) 1997
American Vacuum Society.