Heterogeneity in microcrystalline-transition state: origin of Si-nucleation and microcrystallization at higher rf power from Ar-diluted SiH4 plasma

Das, Debajyoti ; Jana, Madhusudan ; Barua, A. K. (2001) Heterogeneity in microcrystalline-transition state: origin of Si-nucleation and microcrystallization at higher rf power from Ar-diluted SiH4 plasma Journal of Applied Physics, 89 (5). pp. 3041-3048. ISSN 0021-8979

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Official URL: http://jap.aip.org/japiau/v89/i5/p3041_s1?isAuthor...

Related URL: http://dx.doi.org/10.1063/1.1345852

Abstract

Using very high Ar-dilution to the SiH4 plasma, good quality amorphous Si:H films could be obtained at very low rf power. The a-Si:H film, prepared at a very low deposition rate of ~10 Å/min, exhibited a σPh~1×10-4Scm-1PhD~105, a notably wide optical gap of 2.10 eV and a very good stability against thermal annealing effects with reasonable light induced degradation. At higher rf power undoped µc-Si:H films were prepared with a high σD~1×10 -4Scm-1, at a deposition rate of 30 Å/min from <1 sccm of SiH4. Micrograins were identified with several well-defined crystallographic orientations. However, porosity in the grain boundary zone contributed a significant amount of adsorbed effects on the electrical properties. At very high powers, the growth of a columnar network structure was demonstrated. Long-range structural relaxation permitted by the non-rigid and heterogeneous network structure associated with the physical vapor deposition-like growth at the microcrystalline-transition state, has been identified as the origin of nucleation to the Si network and microcrystallization at higher power. It is proposed that Ar in the Ar-diluted plasma provides the energy required for nucleation and grain growth during microcrystallization, and plays an analogous role as atomic H does during chemical annealing in H2-diluted plasma.

Item Type:Article
Source:Copyright of this article belongs to American Institute of Physics.
ID Code:1521
Deposited On:05 Oct 2010 06:42
Last Modified:13 May 2011 09:32

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