We have grown thin films of a-Ge:H and a-Ge:(H, O) by the glow-discharge process, and have used infrared (ir) absorption spectroscopy to study the local bonding of hydrogen and oxygen as a function of the substrate temperature T, and the amount of 02 and/or H&O added to the germane gas mixture in the plasma. The temperature dependence of the ir features associated with monohydride and dihydride groups in a-Ge:H alloys is different in these films, grown at relatively high plasma power, from what has been reported in films of a-Si:H grown from silane plasmas at lower power levels. In particular, dihydride incorporation in these a-Ge:H films displays a distinct temperature threshold, rather than a competition with the monohydride bonding as in the a-Si:H films.The bonding of H and 0 atoms in the ternary alloys a-Ge:(H, O) is also different from what has been reported for the corresponding Si ternary alloys, both in the nature of the local atomic arrangements of the 0 and H atoms, and in the relationship between these bonding environments and the source of the oxygen atoms (02 or H20). These differences in bonding in a-Ge:H and a-Ge:{H,O) films with respect to the corresponding a-Si alloy films reflect differences in both the plasma-phase precursor chemistry and temperature-dependent reactions at the growth surface.
Films of amorphous hydrogenated silicon were deposited from silane and disilane plasmas in a planar diode reactor using rf and dc excitation. Substrate temperature (Ts), total pressure (pT), interelectrode spacing (d), and excitation power (P) were systemically varied. Films were characterized in terms of H content and bonding, optical gap (Eo), ambipolar diffusion length (ld), and performance in p-i-n solar cell structures. The extent of silane polymerization to disilane and higher homologs by homogeneous plasma reactions is indicated as a dominant factor in controlling the composition and properties of a-Si:H deposited form rf- and dc-excited silane plasmas. The optimization of film properties at Ts=230 °C is found to be independently controlled by P, pT, and d inasmuch as they determine the degree of plasma polymerization. Films prepared under conditions promoting plasma polymerization resemble films made from SiH4–Si2H6 mixture feedstocks with nonpolymerizing conditions, exhibiting increased H content, dihydride density, and Eo as well as poorer electronic properties. The similarity of film properties for a variety of rf and dc nonpolymerizing plasmas suggests that the identity of the reactive monomeric film-forming specie(s) is either invariant or noncritical. These films have Eo≂1.7 eV, ld≂0.3 μm, and produce p-i-n solar cells with efficiencies≂7.5%. The roles of homogeneous and heterogeneous processes were investigated. Implications for maximum achievable deposition rates and silane utilization are discussed.
Interactions between radical growth precursors on plasma-deposited silicon thin-film surfaces Dependence of thinfilm microstructure on deposition rate by means of a computer simulationStep coverage in the vacuum deposition of thin metal films
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