Estimation of The Lattice Parameters, Crystallite Size and Internal Micro Strain of Cu1-Xinxse2 Thin Films by Williamson-Hall Method by Korablev Grigory Andreevich* in Determinations in Nanomedicine & Nanotechnology_ Journal of Nanotechnology
Abstract
In
this work, Cu1-xInxSe2 thin films have been grown on heated glass substrates
using chemical spray pyrolysis. Characterizations and compositional analysis of
Cu1-xInxSe2 thin films were obtained by X-ray Diffraction (XRD) and Electron Dispersion Analysis
(EDX). Microstructure parameters as a function of Cu/In and the substrate temperature
(Tsub) in the range of 548K to 623K have been study. Williamson-Hall method has
been used to determine the crystallite size, microstrain. XRD revealed that a
polycrystalline CuInSe2 thin films with the hexagonal structure having
preferential growth along the <002> direction. At the Cu/In ratio
increased, improved of the degree of crystallinity and decrement of both, the
lattice parameters and volume of unit cell. Also, the crystallite size was
found to be increased and decreased with the growth temperature. On the
contrary, the microstrain values were decreasing with the growth temperature
and Cu/In ratio were increasing
Copper
Indium di-Selenide (CIS) is one of the most promising semiconductor materials
used in solar cells in recent years due to its favorable electrical and optical
properties, durability and cost-effectiveness [1-5]. CuInSe2 is a member of the
I-III-VI2 semiconductor group and is present in the chalcopyrite phase of the zinc
blende family [4]. Various methods such as Molecular Been Epitaxial (MBE) [6],
flash vaporation [7,8], multi-source evaporation [9], single-source evaporation
[10], RF-sputtering [11], spray pyrolysis [12,13], Chemical precipitation [14]
and Stacked Elemental Layer (SEL) [15,16] were developed to synthesize CuInSe2
thin films
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