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Science and Engineering Applications 1(3) (2016) 1-8 ISSN-2456-2793(Online)
©JFIPS, India http://www.jfips.com/
Composition dependence structural and optical
properties of the CuInGaSe nanocrystals
Abhay Kumar Singha *, P. Senthamaraib, R. Ganesana
aDepartment of Physics, Indian Institute of Science, Bangalore-560012, India
bDepartment of Physics, Anna University of Technology, Trichy, India
Email: [email protected]
ABSTRACT
This report demonstrates colloidal route synthesis of the Cu24In16Ga4Se56 and Cu24In16Ga7Se53 nanocrystals at
temperature ~ 150 0C. Materials crystallographic phase formations analysis is performed using the X-ray
diffraction, micro-morphology from the Transmission Electron Microscopy and stoichiometric homogeneity by
the energy dispersive X-ray mapping. Modification in the bonds feature and the chemical environment are studied
with the X-ray photoelectron spectroscopy. The optical properties of the materials are described with the help of
UV/Visible, FT-IR transparency and photoluminescence spectroscopy. The synthesized nanocrystals/ particles
size are obtained around ~ 40 nm to ~ 60 nm. The optical energy band gaps are evaluated 1.30 eV and 1.39 eV
for the Cu24In16Ga4Se56 and Cu24In16Ga7Se53 compositions. A higher order photoluminescence is noticed for the
Cu24In16 Ga7 Se53 composition, while the FT-IR transparency is unchanged in these materials.
Keywords: CIGS, Sole gel, Nanomaterials, Semiconducting materials, Crystal morphology, Optical properties.
Received on: 27/8/2016 Published online on: 5 /9/2016
1. INTRODUCTION
More than two decades, chalcogenide based photovoltaic (PV)
modules have been extensively studied due to cost reduction and
high efficiency performance [1-4]. To achieve a reliable, low
cost and high performance PV modules investigators have been
paid attention toward nanocrystalline CuInGaSe (CIGS)
materials [5]. Colloidal CIGS nanocrystals have also attracted
much attention due to the tunability of the optical band gap and
multiple electron-hole pair formation. These two critical
parameters may play a crucial role to improve solar cell
performance. To produce CIGS nano crystals, investigators
preferred to mix Cu, In, Ga and Se elements in intended
stoichiometric ratio with the high boiling point solvent
oleylamine (OLA) [6]. This gives inorganic nanocrystals readily
dispersed within the ligand organic solvent and the final product
is extracted from it. Nanocrystals produced this way can have a
smaller grain size and relatively larger inter- interplaner spacing
owing to presence of organic capping ligand on the surface.
However the smaller grain size and larger interplaner spacing
can limit high density of electrons and holes in the material.
Therefore an appropriate growth of the nanocrystal-grains is a
crucial parameter to get a higher power conversing from the
CIGS material.
Over 15 % efficiency has been reported for the hydrazine
synthesized CIGS nanocrystals modules [7]. It was demonstrated
that the CIGS nano crystals synthesized from this route can be
an efficient absorber material with promising photovoltaic
features. But the use of highly toxic and explosive hydrazine
restricts their commercial utilization. S.H. Mousavi et al. [8] had
demonstrated the colloidal CIGS nanocrystals around 20-40 nm
size with the purity upto 99%.They were commented that choice
of precursor can play an important role in CIGS pure phase
formation. The metallic source precursors led to the formation
mixed phases. While the chloride precursor (except selenium)
could have less impurity phases in CIGS material. Thus the
impurity mainly reflects from the copper selenide phases due to
the fast reaction rate between copper with selenium [9-11].
Therefore, CIGS nanocrystals can also synthesized by using
various solutions based techniques such as microwave assisted
synthesis, solvo thermal synthesis [12], hot injection route [13],
mechano chemical synthesis [14], green synthesis [15], modified
polyol route [16], ambient pressure diethylene glycol based
solution process [9], low temperature colloidal process [10,
11].Here we have synthesized Cu24In16Ga4Se56 and
Cu24In16Ga7Se53 (CIGS) nanocrystals with the aim to see the
effect of gallium and selenium alloying concentrations on the
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nano confined crystals size and their physical properties. The
synthesized nanocrystalline Cu24In16Ga4Se56 and
Cu24In16Ga7Se53 materials physical properties are studied using
the X-ray powder diffraction (XRD), Field Emission Scanning
Electron Microscope- Energy Dispersive X-ray Spectroscopy
(FESEM-EDS) and Transmission Electron Microscopy (TEM)
measurements. The binding energy core levels spectrum is
recorded using X-ray Photoelectron Spectroscopy (XPS). The
UV-Visible and Fourier Transform Infrared (FT-IR)
spectroscopy are used to explain optical properties of the
materials.
2 SYNTHESIS ROOT AND
CHARACTERIZATION
To prepare the CIGS nanocrystals, colloidal route was adopted
under the heating up process in the normal environment.
Precursors copper chloride (CuCl2), indium chloride (InCl3),
gallium chloride (GaCl3) and selenium (Se) compositional
amounts for 2 mg were dissolved into the 15 ml Oleylamine
(OLA) solvent. In the beginning it was noticed prepared solution
in dark blue colour. But with the slow heating (12 h) temperature
upto 160◦C (±10) under a continuous stirring it was changed into
blackish brown colour. The final solution was allowed to cool
down to room temperature. Further, 20 ml methanol and 10 ml
water were slowly incorporated into the solution and again allow
for continuing stirring upto next 12 h at a 60 0C temperature.
Additional methanol and water were formed a gel like substance
within the solution. The formed gel was filtered and washed
several times with methanol and water to reduce byproduct
impurity. The final product was dried at a 150 0C temperature.
The obtained product was crushed in the powder form and it used
for different characterizations. The different stage colours
schematic of the colloidal synthesized CIGS materials is given
in Figure.1.
Figure.1. Schematic solution color representation of the
synthesis process
The XRD measurement in the 2θ range 10 - 90⁰ was performed
from the Rigaku equipment, whereas, the Cu-Kα radiation ( 1.54
Å) source used. Existence of the alloying elementals and their
particles distribution can be verified from the EDS and mapping.
The EDS and elemental mapping were performed from the
ULTRA 55 Karl Zeiss model equipment. To avoid the external
contamination the powder samples were desiccated under at a
vacuum 10-2 Torr and it maintained for the 12 h before performed
the experiment. Further, to minimized the surface charging effect
during the experiment 5 nm gold thin film was deposited on
samples specimen using the ultrathin gold coater equipment.
TEM measurement was performed from the TECHNI G2 T20
equipment. For the TEM grid preparation small amounts of the
samples were dissolved in the 5 ml Dimethylformamide (DMF).
The prepared solutions ultra-sonication was performed upto 5
min. A few drops of the ultra-sonicated solutions were put on top
of the copper grid. Before performing the TEM experiment
copper grid specimens were desiccated for the 24 h under at a
vacuum 10-2 Torr. The XPS characterization was performed
from the high energy resolution AXIS ULTRA-165 instrument.
To produce the photoelectric effect 12 h desiccated samples were
irradiated with a low -energy (~1.5 keV) X-rays under a ultra
high vacuum 1010 torr. The core energy levels spectrum of the
emitted photoelectrons was recorded by the high-resolution
spectrometer.
UV/Visible and reflectivity spectroscopic measurement was
performed from the Sepctro S-600 equipment. The fine powder
of the materials was kept carefully in sample holders and
recorded the UV/Visible absorption spectra in the wave length
range 200 to 1000 nm under a reflectance mode. The PL
characterization was performed in a wave length range 330 to
900 nm from the LabRAM HR equipment. The 325 nm wave
length Argon LASER was used, whereas, the charge coupled
detector (CCD) in backscattering geometry. Spectra were
recorded with the resolution 0.5cm-1. For the FT-IR
measurement fine powders of the samples and KBR chemical
were mixed into the ratio ~5: 95. Then 2.0 mm thick pellets were
made under at a 4 ton load. The FT-IR measurement was
performed in a wave number range 400 to 10000 cm-1 in the
transmission mode by using the Perkin Elmer Spectrum GX.
Spectrum was collected with a resolution of 4 cm-1 in interval of
1 cm-1.
3 RESULTS
3.1. Structural analysis
Crystallographic structure of the described materials is exhibited
in Figure.2 (a, b). XRD pattern of the Cu24 In16 Ga4Se56 material
exhibits the mixed phases of copper indium gallium selenide
(CuInGaSe) and copper selenide (CuSe2). The peak at 2θ
(26.76⁰) is representing CIGS chalcopyrite phase along the [112]
plane. With other relatively weak mixed phase peaks at 29.828,
33.1201, 34.0795, 38.7825, 41.9618, 44.4262, 46.5649, 52.5718,
56.9174 and 60.6789. These weak peaks might be arises due to
inhomogeneous phase mixing of the copper selenide. Figure. 2 b
represents XRD pattern of the Cu24In16Ga7Se53 material. The
Abhay Kumar Singh et al, Science and Engineering Applications 1(3) (2016) 1-8
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prime CIGS characteristic peak is appeared at 27.00 along the
crystallographic plane [112]. Other weak characteristic peaks
are also appearing with the noticeable feature the main CIGS
crystallographic peak [112] shifted toward higher 2θ value for
the Ga 7% containing alloy. The higher intensity of the prime
peak could be correlated to the improved crystalline behavior of
the material. However, weak peaks at 2θ value 30.994, 45.8559
can be correlated with copper selenide secondary phase.
Figure.2 (a, b). XRD patterns of the Cu24 In16 Ga4Se56 and
Cu24In16Ga7Se53 nanocrystals
Materials micro-morphology can be visualized from the
TEM analysis. TEM image of the Cu24 In16 Ga4Se56 is showing
non uniform agglomerated nanocrystals (see Figure.3 (a)) with
the distinguishable grain boundaries. While, the relatively
smaller crystal size and high order agglomeration is appeared
(See Figure.3 (b) ) for the Cu24In16Ga7Se53 composition. This
might be due to higher order phase mixing of the alloying
elements within the configuration. The TEM image analysis
gives the overall particle size around 40 to 60 nm.
Moreover the alloying elemental presence and their distributions
are demonstrated from the EDS and mapping. Figure.4
represents the EDS patterns and their elemental mapping for the
Cu24 In16 Ga4Se56 composition. Existence of the every alloying
elemental peak in their compositional ratio (± 2 %) reveals the
appropriate material configuration.
Figure.3 (a, b) TEM images for the Cu24 In16 Ga4Se56 and
Cu24In16Ga7Se53 nanocrystals
The corresponding elemental mapping in surface cross sectional
area 10 μm is demonstrating their distributions throughout the
configuration. This composition mapping analysis gives the
element copper and selenium particle distributions denser and
uneven throughout the surface. The element gallium particles
distribution is also relatively rarer with the uneven distribution.
While, the element indium distribution seems to homogeneous
throughout the surface area with the lest dense particle
distribution appearance. It could be due to its high order
reactivity and diffusivity with other alloying elements.
Figure. 4. EDS patterns and elemental mapping for the
Cu24In16Ga4Se56 nanoparticles
On other hand Figure.5 is representing EDS pattern and
elemental mapping for the Cu24In16Ga7Se53 composition. EDS
pattern is showing presence of the alloying elements in their
Abhay Kumar Singh et al, Science and Engineering Applications 1(3) (2016) 1-8
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compositional ratio (± 2%).While the alloying elemental
distribution for this composition is exhibiting relatively higher
order diffusion and inclusion within the configuration.
Predominantly the non metallic host selenium, metallic copper
and semi metallic gallium homogenous particle distribution
throughout the surface area reveals their high order reactivity to
each other. This mapping result can also infer in terms of the high
order reactivity of selenium and copper with the gallium, while,
the indium can have a highest reactivity with the individual
alloying element. Therefore, element indium particles
distribution is fewer than other alloying elements even though
less compositional amount of the gallium. Thus the EDS
elemental mapping evidence is demonstrated the higher order
elemental phase mixing for the Cu24In16Ga7Se53 than the
Cu24In16Ga4Se56 nanocrystals.
Figure. 5. EDS patterns and elemental mapping for the
Cu24In16Ga7Se53 nanoparticles
3.2. XPS Interpretation
The XPS measurement has been performed to know the
impact of the alloying elements concentration on the core energy
levels. Figure. 6 (a,b,c,d) is representing XPS spectra of the
copper, selenium, gallium and indium core shell electrons
bonding energies for the under test materials. The Cu24 In16
Ga7Se53 nanocrystals (See Figure.6 a) exhibits the Cu 2p core
energy level splits into 2p3/2 (929.8 eV) and 2p1/2 (949.6 eV) two
peaks having a shift toward higher binding energy side
containing low count value. However, selenium broad strong 3
d5/2 core energy level peak is observed at 52.49 eV, with a
noticeable counts reduction for the Cu24 In16 Ga7Se53
composition (See Figure. 6 b). The valance states for the
selenium can be accessed with the help of past reports [17]. This
XPS outcome is also supporting high order diffusion /or
inclusion of the selenium within the alloys configuration. The
unaltered indium core energy level peaks 3d5/2 and 2p3/2 at 442.3
and 449.9 eV (with a low counts value) is appeared for the Cu24
In16 Ga7Se53 (See Figure. 6 c) composition. Moreover, the core
energy levels binding energies at 1115.6 and 1143 are belongs to
gallium 2P3/2, 1/2 states. The gallium core energy level peak at
1143 is disappeared in the Cu24In16Ga4Se56 composition, while,
it can easily recognize in Cu24 In16 Ga7Se53 composition XPS
profile (See Figure.6 d). The XPS core energy level peak analysis
of the materials has been performed with the reference of carbon
(C1) peak ±2.
3.3. UV-visible interpretation
The optical energy band gap and reflectivity are the
crucial parameter for the photovoltaic materials. Therefore, it is
significant to define the UV-visible optical absorption and
reflection properties. The obtained UV-visible absorption
spectra (solid line) and corresponding Lorentzian fit (circle line)
with optical energy band gap (Eg) Tuac plot (inside profile) for
these compositions is given Figure. 7 (a, b). These materials are
exhibiting a broad UV-visible light absorbance peaks in the
range 400 to 850 nm. The higher order light absorbance is
observed for the Cu24In16Ga7Se53 in comparison to
Cu24In16Ga4Se56 composition. The direct optical energy band gap
(Eg) for the materials is evaluated around 1.30 and 1.39 eV [18-
20].
Moreover, it is well recognized [21-24] that nano
materials overall particle size can also determine from the UV-
visible absorption spectrum. Predominantly, it is appropriate to
describe materials particle size from this approach those
nanoparticles having agglomerated non-homogenous
distribution throughout the configuration [21-24]. Cause it
reflects overall material property instead of the specified location
(or area). Photovoltaic nanocrystalline materials usually do not
possess well defined even grain boundaries. Therefore, it is
customary to describe on-average particle size with the help of
Abhay Kumar Singh et al, Science and Engineering Applications 1(3) (2016) 1-8
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Figure. 6. XPS core level spectra, (a) Copper (b) Selenium (c) Indium (d) Gallium for the Cu24 In16 Ga4Se56 and Cu24 In16 Ga7Se53
nanocrystals
Figure. 7 (a, b). UV-visible absorption spectrum (solid lines), Lorentz fit (circle lines) along with fitting parameter table, optical
energy band gap (Eg) Tuac plot (inside profile); (c). reflectance spectra for the Cu24 In16 Ga4Se56 and Cu24 In16 Ga7Se53 nanocrystals.
Abhay Kumar Singh et al, Science and Engineering Applications 1(3) (2016) 1-8
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Figure. 8 (a, b, c). Photoluminescence (PL) and FT-IR transmission spectrum for the Cu24 In16 Ga4Se56 and Cu24 In16 Ga7Se53
nanocrystals
Figure. 9. Schematic of the reaction mechanism for the synthesized CuInGaSe nanocrystals
(c)
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the UV-visible spectrum Lorentzian fit for the developed
materials. Obtained Lorentzian fit R-square values are 0.815 and
0.699 for the Cu24In16Ga4Se56 and Cu24In16Ga7Se53
compositions. The obtained other parameters (y0, xc, w and A are
in usual meaning) value is given in the table inside the respective
figure. The particle size of the material can be directly related to
inverse of the R value with the help of well established
relationship [25, 26]. Using this approach on average particle
size values 64 nm and 55 nm are obtained for the described
nanocrystalline materials. Here Figure.7 (c) is representing
reflectivity measurement result; both materials have exhibited
the high order reflectivity in the UV-visible wave length range.
This is also consisting with the photovoltaic material essential
criteria reflectivity should be low in UV-visible wave length
range.
3.4. Photoluminescence and FT-IR interpretation
To know the optical quantization behaviuor in these
materials, we were performed the Photoluminescence (PL)
measurement in the wave length range 400 nm to 800 nm. Both
materials are exhibiting a strong PL single (See Figure. 8 (a, b))
at a room temperature. This reflects under test materials have a
high order nanoparticles confinement within the quantized
energy levels. Significantly it gives material Cu24In16Ga7Se53 has
a stronger PL property than the Cu24In16Ga4Se56. Further, to
explore the IR optical properties of these materials we have
performed FT-IR measurement in the wave number range 400
cm-1 to 4000 cm-1 (see Figure. 8 c ). Both materials have exhibited
IR transmission spectra with a low transparency percentage in
the wave number range 600 to 3200 cm-1. Both materials IR
spectrum are exhibiting a small multi phononic jump peak above
the 3200 cm-1 wave number range. The two combined functional
absorption groups are also appeared at 1699 and 2844 cm-1. This
may be due to adopted non vacuum drying process of the
samples. Besides materials have a good IR transparency in the
MID-IR range they could not be considered a promising
candidate for the IR application, cause, low transparency
percentage as compare to other existing materials.
4. DISCUSSION
Nanocrystals formation in aforesaid materials could be
interpreted with three steps mechanism under the followed
heating up process. The schematic of the mechanism is given in
Figure.9. Due to less reaction temperature requirement the CuSe2
phase can be formed first at the low temperature. It could be
become only from the OLA– copper complex decomposition.
Resulting it can be released the monomers containing Cu+ ions
at low reaction temperature (~1000C) in a shorter time period. As
well as the reactivity of the OLA–copper complex increases and
reach at a much higher temperature then OLA–In and Ga
complexes can react. Therefore, the monomers containing Cu+
ions can react with the Se ions. As a consequence dissolution of
the Se in OLA can be increased with a reduction of Se powder
in colloidal configuration and it results the CuSe2
nanocrystallites phase formation [20]. It is well defined the
reactivity of the Se depends on the reaction temperature and
reduction ability of the ligand. Therefore, at a low reaction
temperature (~1000C) materials may form the CuSe2 phase due
to weak reduction ability of the OLA with the Se powder. In the
second step it can deliver In+ ions monomer when the reaction
temperature in between the 1000C to 1500C. Therefore the
thermally enhanced decomposition of the OLA–In complex
increases slowly and reacts with Se2 ions. Results the In-rich
selenide shells on the surfaces of CuSe2 nanocrystallites through
surface nucleation. Then CuSe2 nanocrystallites can react with
the inner diffused In ions and form CuInSe2 phase. In the final
step; where temperature ≥ 1500C with continuous stirring the
thermal decomposition of the OLA-Ga complex is occurred
resulting the CuInGaSe nanocrystals through the surface
nucleation reaction mechanism [27,28].
Thus the physical property modifications in these
materials could be correlated with these words; reduction and
increment of the selenium and gallium alloying amounts alter the
properties of the materials due to increase in the rate of reaction;
by making the more metalloid and less non metallic bonds within
the configuration [29, 30, 31]. The incorporation of the
additional amount of gallium as cost of selenium can affect the
chalcogen chains and rings within the configuration. During the
long chemical processing alloying element particles interacts
strongly through breaking the individual bonds and the
combined effect reduced the crystals/particles size with an
induced strong quantum confinement at the nano level. The
colloidal interaction in between the gallium and copper can also
play a key role in crystals/particles size modifications owing to
their high metallic nature reactivity. However, alloying element
indium can substantially contribute to homogenize the
configuration structure due to its recombination blocking ability.
5. CONCLUSIONS
In summary, authors have discussed the colloidal synthesis and
physical properties of the Cu24In16Ga4Se56 and Cu24In16Ga7Se53
composition nanocrystals. The obtained experimental evidences
have revealed low temperature (≥ 1500C) colloidal route
synthesized materials physical properties is varying with the
alloying elements concentration. TEM and Lorentzian fit have
demonstrated the agglomerated phases with the nanocrystals
average size ≤ 64 nm for the Cu24 In16 Ga4Se56 composition.
While, the Cu24In16Ga7Se53 composition has a rather
agglomerated homogeneous distribution of the nanocrystals with
the reduced size around ≤ 55 nm. The reduction in the
Abhay Kumar Singh et al, Science and Engineering Applications 1(3) (2016) 1-8
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nanocrystalline size and homogeneous distribution has affected
the binding energies of the elemental core levels, UV-visible
absorption, reflectivity, optical energy band gap, PL and FT-IR
transparency. Therefore, the experimental evidence
demonstrates element gallium has optical energy band gap
tunability aptitude through the physical modifications in
Cu24In16Ga4Se56 and Cu24In16Ga7Se53 composition nano-
materials. Hence Cu24In16Ga7Se53 composition nanocrystalline
material can have a superior prospect for the photovoltaic
application in comparison to Cu24 In16 Ga4Se56 composition.
ACKNOWLEDGEMENT
AKS thankful to the Centre for Nano Science and Engineering
(CeNSE)-IIsc, for the materials characterizations.
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