SnS-based thin film solar cells: perspectives over the last 25 years
Transcript of SnS-based thin film solar cells: perspectives over the last 25 years
SnS-based thin film solar cells: perspectives over the last 25 years
Jacob A. Andrade-Arvizu1 • Maykel Courel-Piedrahita1 • Osvaldo Vigil-Galan1
Received: 30 January 2015 / Accepted: 4 April 2015
� Springer Science+Business Media New York 2015
Abstract New types of thin film solar cells made from
earth-abundant, non-toxic materials and with adequate
physical properties such as band-gap energy, large ab-
sorption coefficient and p-type conductivity are needed in
order to replace the current technology based on
CuInGaSe2 and CdTe absorber materials, which contain
scarce and toxic elements. One promising candidate ab-
sorber material is tin monosulfide (SnS). The constituent
elements of the SnS film are abundant in the earth’s crust,
and non-toxic. If this compound is used as the absorber
layer in solar cells, high efficient devices should be fabri-
cated with relative low cost technologies. Despite these
properties, low efficiency SnS-based solar cells have been
reported up to now. In this work, we present a review about
the state of the art of SnS films and devices. Finally, an
analysis about different factors that are limiting high effi-
ciency solar cells is presented.
1 Introduction
The production of solar cells with low cost, high efficiency
and by means of environmental friendly processes is the
current challenge for terrestrial applications. Thin film
photovoltaics (TFP) technology, known as second gen-
eration of solar cells, emerged to meet some of these ex-
pectations. Themassive use of solar cells requires increasing
the conversion efficiency of the devices and effective
lowering of the manufacturing costs [1]. It goes without
saying that thin films have the potential to revolutionize the
present cost of photovoltaic devices as alternative to silicon
technology [2]. Additionally, in terms of cost and efficiency,
the second generation of solar cells could be seen as a future
resource for sustainable energy.
Many have been the attempts made over the past century
until today for searching non-toxic and cost-effective new
materials with adequate properties for photovoltaic applica-
tions. Certainly, the developments of binary and ternary ma-
terials, such asGalliumArsenide (GaAs), CadmiumTelluride
(CdTe), Copper-Indium-Gallium-Selenide (CIGS), etc., have
created pathways compared to the first generation solar cells
technology, due to the favorable properties and simplicity in
their synthesis. Lately, the most advanced materials for
making thin film solar cells are based on the use of CdTe or
CIGS as absorber layer materials [3]. However, problems
related to toxicity [4–7] and scarcity of someof the constituent
elements of these compounds have been reported as issues to
overcome, in a mass production [8].
To achieve cost-effective thin film solar cells for large-
scale production, the absorbing semiconductor material
used in the device needs to satisfy many requirements.
First, the constituent elements should be inexpensive, non-
toxic and abundant in the earth’s crust. Second, to obtain
high conversion efficiencies, the material should have ap-
propriate optical and electrical properties such as a suitable
optical band gap, a high optical absorption coefficient, a
high quantum yield for excited carriers, a long minority
carrier diffusion length, and a high minority carrier lifetime
(a low recombination velocity) [9]. Compounds such as tin
sulfide (SnS) have been considered as materials that can
meet these requirements; however, far lower efficiency
values have been reported in solar cells based on SnS as
absorber.
& Maykel Courel-Piedrahita
1 Escuela Superior de Fısica y Matematicas-Instituto
Politecnico Nacional (IPN), C.P. 07738 Mexico, D.F.,
Mexico
123
J Mater Sci: Mater Electron
DOI 10.1007/s10854-015-3050-z
In material science, efforts persist on finding new
sustainable materials. New approaches have considered
kesterite compounds for solar cell applications. However,
several problems have been identified as principal hurdles
to boost solar cell performance, reaching efficiencies
lower than 13 % [1, 10–14]. On the other hand, among
many semiconducting metal Chalcogenides, tin sulfides
have attracted extensive interest due to its physical and
chemical properties for solar energy conversion, espe-
cially by its photoconductive character [15, 16]. Despite
this material has been widely studied; as far as we know,
there is no report that embraces results obtained for both
SnS physical properties, and its application in solar cells.
Besides, the main critical aspects to improve both mate-
rial properties and solar cell performance have not yet
been identified.
In this work, a review about SnS properties and its ap-
plication results in thin film solar cells is presented. The
most used techniques and results about SnS thin film pro-
cessing are presented. In order to improve SnS-based thin
film solar cell performance, several hurdles are identified.
Finally, a critical discussion about a further solar cell ef-
ficiency improvement is presented.
2 SnS: a potential absorber for thin film solar cellapplications
2.1 Brief history
The tin sulfide (SnS) compound was first reported by a
German mineralogist Robert Herzenberg in the year 1932
[17], being this the main reason for the mineral to be
recognized as herzenbergite, also known as: Kolbeckine.
Since then, many are the available studies on the struc-
tural, optical and electronic properties as well as its pe-
culiarities with synthesis parameters and fabrication
techniques. In this regard, the p-T-x diagram for the Sn-S
system was then determined in the early 60 s by Albers
et al. [18] especially in the region of the SnS compound.
Also, this investigation group showed that the existence
region of solid SnS lies entirely with a high degree of
probability at the excess sulfur side. This diagram also
results to be quite helpful for the understanding of the
feasibility of Tin binary sulfides formation such as SnS,
and SnS2 even at low temperatures and with a suitable
Sn/S ratio. Some years later, in 1979, an exhaustive report
on various SnS minerals was stated by Kissin and Owens
[19]. After almost 25 years later, Dittrich et al. [20]
studied the sulfo-salts emphasizing their potential impor-
tance in the field of photovoltaic devices.
2.2 IV–VI semiconductors: the tin sulfides family
In nature, it is found that tin sulfide compounds exist in a
variety of phases such as: SnS (Orthorhombic/Zinc Blen-
de), SnS2 (Hexagonal/Trigonal), Sn2S3 (Orthorhombic),
and Sn3S4 (Tetragonal), as well as in numerous polysulfide
anions due to bonding characteristics of tin and sulfur.
Among them, only SnS, SnS2 and Sn2S3 are discrete
phases. The oxidation state may take ?2, ?4 for tin and
-2,-1, 0 for sulfur. The tin sulfide chemistry is then further
enriched by the catenation ability of sulfur. In addition, it
has been observed by Jiang and Ozin [21] that other metallic
and non-metallic elements can be incorporated into the tin
sulfide structures to yield ternary and quaternary materials or
the successful doping of the compound.
Besides, all these binary compounds behave as semi-
conductor materials, and exhibit n or p type conductivity
depending on the tin concentration. Among the tin
chalcogenide thin films, SnS and SnS2 are the most im-
portant ones because of its suitable opto-electronic prop-
erties for photovoltaic applications. Due to optimum band
gap, high absorption coefficient and p-type conductivity,
SnS results to be a suitable candidate for absorber layer in
thin film solar cells whereas SnS2 for window layer be-
cause of the wider band gap and n-type conductivity. In
fact, SnS2 has been considered as an alternative non-toxic
buffer layer to CdS.
Therefore, three of these binary compounds based on the
Sn–S system (SnS, SnS2, and Sn2S3) result to be interesting
from a technological point of view. The Sn2S3 is classified as
a type I mixed valence compound (II and IV valence) with a
semiconductor behavior, whose optoelectronic properties
are dependent on the crystalline structure and stoichiometry.
These compounds could be used to build photovoltaic p–n or
p–i–n structures with a conversion efficiency of about 25 %
according to the Loferski’s limit [22]. These structures
would be low-cost devices, because the materials involved
are cheap, nonstrategic, and abundant in nature. In addition,
Sn2S3 is a semiconductor material that appears to be suitable
for preparing near-lattice-matched heterojunctions in sys-
tems such as Sn2S3/CdTe, Sn2S3/GaSb, Sn2S3/AlSb, etc.
These systems have applications in the detection and gen-
eration of infrared radiation [23]. Table 1 displays structure,
lattice constants, band gap value and conductivity type for
the tin sulfide family. Among the different phases, SnS with
direct band gap shows adequate properties to be used as an
absorber due to its suitable band gap *1.4 eV and p-type
conductivity. On the other hand, SnS2 compound with hex-
agonal structure is characterized by a high band gap value
(2.2 eV) with direct transitions and n-type conductivity
making it attractive for buffer layer applications.
J Mater Sci: Mater Electron
123
2.3 Tin sulfide (SnS) as a proper candidate
for second generation solar cells
As remarked in the previous section, one promising ma-
terial for absorber layer in thin film solar cells is the metal
monochalcogenide tin monosulfide (SnS). This material
has a near optimum energy band gap and exhibits an am-
photeric character promising the possibility of grain
boundary passivation. Not only does SnS consist of
relatively abundant elements but large scale production
processes already exist for producing thin films of tin and
for converting metals into the corresponding sulfur com-
pounds using a range of chemical, physical and sulfuriza-
tion processes. Some of the main properties of SnS
compound are presented in Table 2.
In addition, this compound is chemically stable in acidic
as well as alkaline media due of its amphoteric character
[53]. According to the Shockley–Queisser criteria [54], a
maximum efficiency up to 33 % could be achieved for this
material (for a direct band gap energy of approximately
1.3 eV). Nevertheless, this result seems to be a very first
rough approximation. On the other hand, another possible
estimation for conversion efficiency limit could be eluci-
dated for different materials as a function of their optical
band gaps from the theory contained in the Loferski dia-
grams [22]. Under this approach, an efficiency value higher
than 24 % was obtained. This result along with the prop-
erties reported in Tables 1 and 2 emphasize the acceptance
of SnS as a good candidate for an absorber material. SnS
crystals present natively p-type conductivity due to the
small formation enthalpy of tin vacancies, which generate
shallow acceptor-like vacancy defects [55]. Amorphous
and crystalline SnS films show a direct band gap of:
1.0–1.65 eV and an indirect of 1.0–1.45 eV [56] with an
absorption coefficient of around 104 cm-1 which means an
absorption length about 1 lm. Besides, SnS compound has
shown an inert surface with few surface states [40, 56].
This might reduce the carrier recombination losses due to
defects at p-n junctions and at grain boundaries [31].
Furthermore, Hofmann [57] have considered the SnS-
orthorhombic structure as pseudo-tetragonal one. Every Sn
atom stays surrounded by three S atoms forming bond
angles around 90�. SnS has a unit cell with lattice pa-
rameters as presented on Tables 1 and 2. On the other
hand, a comparative study on binary metallic chalcogenide
semiconductor materials demonstrated that the ionicity and
transverse charges increased in the order of GeS ? Ge-
Se ? SnS ? SnSe [58, 59]. Ettema et al. [60] reported the
existence of SnS in two different forms such as a-SnS and
b-SnS with similar charge distribution. They suggested that
the a-SnS is a low temperature phase compound with lower
symmetry than the high temperature b-SnS phase. In ad-
dition, a-SnS phase shows a higher band gap (indirect
1.6 eV, direct 1.8 eV) respect to the b-phase. On the other
hand, some properties of the films related with lattice
mismatch, defects, and an improvement in the grain size
could significantly improve the efficiency of the device
[40].
3 SnS thin film fabrication
3.1 Routes of synthesis
In the last three decades, thin films of SnS have been
synthesized by means of diverse physical and chemical
routes; among them, Table 3 shows the most representative
synthesis pathways. Each method has its own advantages
and disadvantages in the production of homogeneous and
defect-free thin film materials. New ways of synthesis
routes are being evolved in order to produce controlled size
and shape of desired morphology. In general, the measured
properties of SnS samples depend on the synthesis route. A
brief description of each method is described below.
3.1.1 Physical routes
3.1.1.1 Two-step process The basic principle of this
synthesis route consists of the sulfurization of thin metallic
tin precursor layers. Reddy et al. [61] reported a detailed
study of the structural properties of the SnS thin films
deposited using the TSP. Here, the sulfurization process
Table 1 Structure, lattice constants, band gap value and conductivity type for the tin sulfide family
Material Structure a (A) b (A) c (A) EG (eV) Type of conductivity References
SnS (tin monosulfide) Orthorhombic 3.64 11.21 3.99 1.35 (direct)/
1.1 (indirect)
P/N [24–26]
SnS2 (tin disulfide) Hexagonal 3.64 3.64 5.90 2.22 (direct) N/P [27]
2H-SnS2 Orthorhombic 3.64 3.64 5.89 – P [28]
Sn2S3 (tin sesquisulfide) Orthorhombic 8.84 14.02 3.74 2.05 (direct)
0.53 (indirect)
N [29]
J Mater Sci: Mater Electron
123
was carried out at different temperatures (100–400 �C) in a
sulfur rich environment. Some years later, Gordillo et al.
[64] synthesized SnS:Bi thin films out of this technique.
The characterization studies revealed that the SnS:Bi films
tend to grow with a mixture of the SnS and Bi2S3 phases. It
was also found that the SnS:Bi films exhibit an absorption
coefficient [104 cm-1 and a direct energy band gap
ranging from 1.37 to 1.47 eV, indicating that this com-
pound shows the required optimal properties for an ab-
sorber layer in thin film solar cells.
3.1.1.2 Atomic layer deposition Homogeneous and ultra-
thin films of various materials can be coated on a variety of
substrates by means of this route. SnS was deposited by
Table 2 Main properties of SnS compound
Type of property References
Crystal structure Orthorhombic Herzenbergite polycrystalline
(2/m 2/m 2/m)
Also: hexoganol (Wurtzite) and cubic (Sphalerite) crystal
forms which are less stable than herzenbergite at room temperature
[30, 31]
Space group Pnma, Cmcm, Pbnm [31–33]
Atoms/cm3 4.15 9 1026 [30]
Unit cell volume (A3) 192.67 [33]
Atoms per unit cell 4
Molecular weight (g) 150.78
Density (g/cm3) 5.08 [34]
Lattice constants (A) a b c [31, 35]
3.64 11.21 3.99
Effective hole masses m (||a) m (||b) m (||c) [34]
0.2 m0 0.2 m0 1.0 m0
Conductivity type p-type: Stoichiometric [36–38]
n-type: S vacancies–Sb doped
Intrinsic resistivity (X cm) 13–20 [31, 35]
Effective electron density (cm-3) 6.3 9 1014–1.2 9 1015 [35, 39]
Effective hole density (cm-3) 1018 [35]
Hole mobility (Hall Mobility) (cm2/Vs) T = 300 K T = 2 9 103 K [31, 35]
50–90 77
Work function (eV) 4.2 [35, 40]
Binding energy (eV) S2p3/2 S3p5/2 [31, 35, 41]
161.4 485.3
Dielectric constant e(0) e(0) [34, 42]
E||a : 32 E||a : 14
E||b : 48 E||b : 16
E||c : 32 E||c : 16
a (cm-1) (absorption edge) 104 [24]
Refraction index 3.52 [24]
Band gap energy (eV) Egdirect Egindirect [24, 26, 40, 42–51]
1.35
Reported in the range
of values: 1.0–1.65
1.1
Reported in the range
of values: 1.0–1.45
Debye temperature (K) 270 [52]
Linear thermal expansion coefficient (K-1) 2.8 9 10-7 [34]
Heat capacity (J/mol K) Cp @300K Cp @80K [34]
45 29.3
Melting point (K) 1154 [31]
J Mater Sci: Mater Electron
123
this technique using sequential exposures of Sn(II) 2,4-
pentanedionate (Sn(acac)2)and H2S. It has been shown that
using the ALD method, the growth rate of SnS thin films
stayed independent of substrate temperature in the range of
125–225 �C. X-ray fluorescence studies showed that Sn/S
atomic ratio was *1.0 for the SnS films. Also, XPS
measurements revealed that the films contained oxygen
impurities at 15–20 % atomic after air exposure. The films
had a band gap of *1.87 eV which was higher than the
value of the bulk (*1.3 eV) [65].
3.1.1.3 Co-evaporation Polycrystalline SnS thin films
have been grown on glass substrates using this procedure
involving chemical and physical reactions between the si-
multaneously evaporated precursor species. Thin films of
SnS were prepared by this method ranging from 200 to
400 �C. The chemical composition of the SnS films results
to be regulated by controlling the evaporation temperature
and/or the amount of the S and Sn evaporated masses. It
was found by Cifuentes et al. [66] that using an adequate
set of deposition parameters; it is possible to get tin sulfide
films in the SnS phase with orthorhombic structure (111) or
in the SnS2 phase with tetragonal structure (001). In this
paper, it is also reported that the refractive index of the SnS
films is significantly greater than that of the SnS2 films.
On the other hand, Koteeswara et al. [67] deposited thin
films at a temperature of 300 �C. A high crystalline quality
along with a dominant SnS phase (040) films were ob-
tained. They also reported that the growth rate of the layers
was directly proportional to the temperature. Nearly
stoichiometric, low-resistive and single-phase SnS films
with an optical band gap of 1.37 eV were synthesized and
reported which could be used as an absorber in the fabri-
cation of thin film heterojunction photovoltaic devices.
3.1.1.4 Close-spaced sublimation/close-spaced vapor
transport As far as we know, Yanuar et al. [68] reported
for the first time the synthesis of SnS thin films by the
CSVT method. The as-grown films showed natively p-type
conductivity with a hole concentration of 1017cm-3, an
energy band gap of 1.32 eV, an absorption coefficient of
104 cm-1 and a low Hall mobility of 3.73 cm2/Vs. The
films also showed a single phase and an excellent crys-
talline quality with prismatic shaped crystallites of about
1 lm. Years later, Xiao et al. [70] synthesized SnS by the
CSS technique at higher temperatures (650 and 720 �C)showing that with the increase of the source temperature
the grain sizes increased around 650 %. They also reported
the values for the direct band gap energies of 1.21 and
1.15 eV for each temperature, respectively.
3.1.1.5 Hot wall vacuum deposition Thin films and
nanorods of Sn1-xPbxS (0.00 B x B 0.45) with
orthorhombic (001) crystal structure and c-axis oriented
perpendicular to the substrate surface presenting a strong
(004) oriented peak were synthesized by the HWVD
method. The as-deposited films were pin-hole free and
strongly adherent to the surface of the substrate. Sn1-xPbxS
layers appeared grey in color and the evaluated thickness
varied from 2.0 to 4.0 lm [71, 72].
3.1.1.6 Molecular beam epitaxy A systematic investiga-
tion of optoelectronic properties of SnS grown by MBE
technique is reported by Wang et al. [73]. Energy band
Table 3 Physical and chemical routes used in the deposition of SnS thin films
Physical routes Chemical routes
Synthesis route References Synthesis route References
Two-step process [61–64] Brush plating [82]
Atomic layer deposition [16, 65] Chemical bath deposition [44–49, 78, 83–95]
Co-evaporation [63, 66, 67] Chemical vapor deposition [96–99]
Close-spaced vapor transport/
close-spaced sublimation
[68–70] Pulsed CVD [100]
Hot wall vacuum deposition [71, 72] Plasma-enhanced CVD [101]
Molecular beam epitaxy [73] Dip deposition [102]
Thermal evaporation [42, 43, 74–78] Electron beam evaporation [103]
Vacuum evaporation [24, 25] Electrodeposition [26, 50, 51, 95, 104–120]
Rf—sputtering [79, 80] Multilayer-based solid-state reaction [121]
Physical vapor deposition [81] Successive ionic layer adsorption and reaction [122–124]
Spray pyrolisis [23, 35–38, 63, 125–139]
J Mater Sci: Mater Electron
123
simulation indicates that SnS had an indirect bandgap of
0.982 eV. Furthermore, the report indicates that elemental
Cu could be used as a p-type dopant for the absorber ma-
terial. Besides, the authors have noticed a significant re-
duction in the rocking curve FWHM over the existing
published values. Also, a crystallite size in the range of
2–3 lm was observed.
3.1.1.7 Radio frequency sputtering In the IEEE confer-
ence of the year 1994, Guang-Pu et al. [140] reported the
preparation of SnS thin films by RFS method for the first
time. The chemical composition, crystal structure, optical
and electrical properties were also reported in this work.
Besides, a critical discussion about the relationship be-
tween the SnS film properties and the sputtering parameters
was also added. Using Sb as a dopant and combining it
with thermal annealing at elevated temperatures (about
400 �C); n-type SnS thin films were obtained. Years later,
Hartman et al. [139] sputtered films with a SnS target by
means of using argon plasma. They have found that the
resistivity, stoichiometry, phase, grain size, shape, band
gap, and the optical absorption coefficient can be varied by
modifying argon pressure for a fixed deposition time in
these films. They have also reported values for the indirect
band gap of 1.08–1.18 eV.
By the year of 2014, Xu et al. [79] utilized polyamide
substrates to improve flexibility of SnS thin film hetero-
junctions. ZnO/SnS heterojunctions were deposited by
magnetron sputtering and their properties were studied.
Post annealing of the films enhanced the crystalline quality
of the compound as observed by other techniques. With a
preferential orientation along the (040) plane and grain
sizes of 18 nm, the compositions of as-deposited and an-
nealed flexible SnS thin films were close to the stoichio-
metry of SnS. The fabricated ZnO/SnS flexible
heterojunctions showed rectifying properties with a recti-
fying ratio of 6.85 and a diode ideal factor of 1.23.
3.1.1.8 Thermal evaporation Nahass et al. [43] have
synthesized SnS thin films by this physical deposition
route. In this work, the authors investigated the structural
transformation after an annealing process at the tem-
perature range of (160–300) �C. Additionally, an exhaus-
tive report on the various optical properties of SnS films
was also included in this paper. The substrate often plays a
critical role in determining the properties of the deposited
film, especially when the deposition technique is thermal
evaporation. Devika et al. [41] have investigated the effect
of annealing on the composition, crystal structure, surface
features and opto-electronic properties of thermally
evaporated SnS thin films and found that with annealing
temperature increase, the composition of the film changed
due to re-evaporation of Sulfur. The SnS structure in the as-
deposited and annealed films remained orthorhombic. With
an increase in substrate temperature, the grain size and the
surface roughness were reduced. Also, the electrical re-
sistivity decreased. As a peculiar observation, the films
annealed at 100 �C showed some unusual features com-
pared to those annealed at other temperatures. Miles et al.
also deposited SnS thin films on glass and onto SnO2:
coated glass substrates, by using thermal evaporation with
the aim of optimizing the properties of the film for using in
solar cells. In particular, they investigated the effects of
source temperature, substrate temperature, deposition rate
and film thickness on the chemical and physical properties
of the films [76].
3.1.1.9 Vacuum evaporation There are few reports of
SnS thin film synthesis by the direct VE of tin sulfide
compound powder. Noguchi et al. [25] prepared tin sulfide
(SnS) films by the vacuum evaporation technique. As-
grown SnS films showed p-type conduction with a resis-
tivity of the order of 13–20 X cm, a carrier density of
6.3 9 1014–1.2 9 1015 cm-3, and Hall mobility values in
the range of 400–500 cm2/Vs. Devika et al. [24] discussed
the influence of annealing on physical properties of
evaporated SnS films and observed that desulfurization
took place owing to the re-evaporation of S from SnS films.
They also showed that at higher annealing temperatures,
defragmentation of grain size could be observed. Devika
and collaborators also studied the influence of substrate
temperature on surface structure and observed that films
grown at higher substrate temperatures showed a large
grain size distribution compared to that at room tem-
perature. Besides, they observed an indirect band gap for
all the prepared SnS films lying somewhere between 1.37
and 1.42 eV.
3.1.1.10 Physical vapor deposition The PVD method
describes a variety of vacuum deposition methods used to
deposit thin films by the condensation of a vaporized form
of the desired material. Revathi et al. [81] deposited SnS
films onto different substrates such as glass, ITO, and Mo-
coated glass. The role of the substrate was then analyzed
depending upon the compositional, microstructural and
photoelectrochemical properties of the SnS films.
Orthorhombic structures with nearly stoichiometric ele-
mental compositions (Sn/S ratios of *1.01) were observed
for all the substrates. Particularly, SnS films deposited on
ITO and Mo-coated glass substrates, exhibited (040) plane
as preferred orientation whereas the films deposited on
glass showed (111) plane as predominant. Also, the Raman
spectra showed SnS single phase contribution. The p-type
conductivity and high photoresponse for films deposited on
the ITO substrate suggested them as a good candidate for a
solar cell absorber.
J Mater Sci: Mater Electron
123
3.1.2 Chemical routes
3.1.2.1 Brush plating Thin films of polycrystalline
orthorhombic (040) p-SnS were brush plated onto tin oxide
coated glass substrates from aqueous solution containing
SnCl2 and Na2S2O3 [82]. The variation of space charge
capacitance, with applied potential (Vapp), was recorded for
the PEC cell with a p-SnS/Fe3?, Fe2?/Pt structural system.
Also, the spectral response of the PEC cell formed with the
SnS photoelectrode was studied and reported. The crys-
tallite size was reported to be in the range of 0.3–0.7 lm.
3.1.2.2 Chemical bath deposition (CBD) Numerous re-
ports are available about the fabrication of SnS thin films
using different precursor solutions, which render Sn2? and
S2- ions for the synthesis of the thin films. CBD is a simple
and very popular technique for thin film deposition, espe-
cially for the deposition of metal chalcogenide thin films.
Pramanik et al. [83] developed this technique for the syn-
thesis of SnS thin films on glass substrate at room tem-
perature. The deposited films were amorphous and
presented n-type conductivity with an optical band gap of
1.51 eV. Two years later, in 1989, Ristov et al. [84] syn-
thesized p-type tin sulfide thin films from SnCl2 and Na2S
precursor salts. An interesting observation was revealed
when annealing this film several hours. Above 280 �C the
conductivity changed to n-type without any detectable
change in the composition, but annealing for a longer time
(over 24 h) changed the composition to SnS2. For higher
temperatures (300–400 �C) in open air, oxidation of the
films was observed, changing its composition to SnO2. In
the next year, Engelken et al. [85] dissolved sulfur in
propionic acid, after which SnCl2�2H2O, potassium glu-
conate or tartaric acids were added. The solution was
heated from room temperature to 90 �C and the bath turned
in a yellowish color, after which the color changed to slate
grayish within a 60 s period. After 30 min, SnS films of
1 lm thickness were obtained. One year later, Lokhande
et al. [86] reported the procedure for depositing various
metal chalcogenide thin films including SnS by employing
CBD technique. By the same year, a much simplified
technique for preparing good quality SnS films was re-
ported by Nair et al. [87]. They were able to deposit uni-
form p-type films with thicknesses up to 1.2 lm. These
films exhibited slight photosensitivity as well. In the same
year and by the same group, the application of these SnS
films as tubular solar collectors owing to its high ab-
sorbance was accentuated [78]. Nair et al. [88] reported the
deposition of good-quality thin films of SnS, CdS, CdSe,
etc., establishing the possible phase transformation from
SnS to SnO2. Thin tin sulfide films deposited by Tanu-
sevski [89] were polycrystalline with an orthorhombic
structure. These films were thermally treated in argon
atmosphere at 300 �C showing an increment in the crys-
tallinity degree. The value of 1.38 eV for the optical
bandgap was determined for the direct transitions and
presented no change after the thermal treatment. From the
red edge of the photoconductivity spectrum, a band gap of
Eg(ph) = 1.24 eV was determined. An impurity level with
an activation energy of 0.39 eV and a thermal band gap of
Eg(T) = 1.19 eV were determined by the temperature de-
pendence of the dark resistance of the films. SnS thin films
with porous structure were synthesized by Lei et al. [90] on
glass using Triethonalamine (TEA), Thioacetamide,
SnCl2�H2O and aqueous ammonia as reactants and aqueous
NH4Cl solution as buffer. All the samples were polycrys-
talline with an orthorhombic structure. The properties of
these porous structures are in principle more suitable for
third generation photovoltaic devices. Two years later,
Akkari et al. [92] investigated the influence of TEA con-
centration on the properties of SnS films for a post-opti-
mization of the deposition parameters. These films
exhibited an orthorhombic structure and a direct band gap
about 1.65 eV. Hankare et al. [44] deposited SnS films on
non-conducting glass substrate at room temperature. The
thin films resulted to be uniform, well adherent and
brownish colored. The optical band gap of the samples was
1.0 eV. The films exhibited p-type conductivity with an
activation energy of 0.62 eV.
By multi-deposition runs, SnS thin films with a Zinc
Blende structure were synthesized by Akkari et al. [46].
The precursors were aqueous solution containing 30 ml
TEA, 10 ml Thioacetamide, 8 ml Ammonia solution and
10 ml of Sn2? (0.1 M). The crystallinity of the films was
improved with film thickness and the band gap energy was
about 1.76 eV for a film prepared after six deposition runs.
By the same year (2010), Guneri et al. [47] deposited SnS
on glass substrates by keeping the bath for 24 h. The films
were nearly stoichiometric (Sn/S = 1.18) and presented
p-type conductivity. Its resistivity and mobility values were
found to be 2.53 9 105 X cm and 8.99 9 105 cm2/Vs,
respectively. Besides, an activation energy of 0.527 eV
was calculated. Optical band gap values of direct and
indirect transitions were estimated to be 1.37 eV and
1.05 eV, respectively. In a following work, they reported
the effect of deposition time on the structural, electrical and
optical properties of SnS thin films at different deposition
times (2–10 h) at 60 �C [48]. All the deposited films were
polycrystalline in nature and presented an orthorhombic
structure with small crystal grains. Despite this, the mi-
crostructures presented substantial changes with the depo-
sition time and were nearly stoichiometric. Hall
measurements showed that the obtained films had p-type
conduction and resistivity values of SnS films also changed
with deposition time. Band gap measurement indicated that
for allowed direct, allowed indirect, forbidden direct and
J Mater Sci: Mater Electron
123
forbidden indirect transitions, band gap values varied in the
range 1.30–1.97, 0.83–1.36, 0.93–1.49 and 0.62–1.23 eV,
respectively for these set of samples. The influence of the
pH value (pH 1.5–3.5) in this technique on the growth and
properties of SnS thin films were investigated by Kassim
et al. [49]. The authors obtained relatively uniform grain
size, good coverage and thicker films for lower pH value
such as pH 1.5. Band gap values were found to be
1.2–1.6 eV for the films deposited under various pH
values.
Over 3 years later, Safonova et al. [93] showed that SnS
films of 100–500 nm can be deposited onto ZnS and CdS
substrates using tin chloride and thiosulfate as the precur-
sors. The deposition was carried out at 25 �C. In a single
deposition way, film thicknesses in the range of
110–170 nm were achieved. On the other hand, by using
two more successive depositions, film thicknesses in the
range of 450–500 nm were obtained.
3.1.2.3 Chemical vapor deposition Price et al. [97] de-
posited SnS films employing atmospheric pressure CVD
technique using Tri-n-Butyltin Trifluoroacetate and H2S as
precursors at 350–600 �C under a nitrogen atmosphere. An
exhaustive Raman analysis was performed on the samples
and the results were discussed. Barone et al. employed
Aerosol assisted CVD to deposit SnS thin films. In this
work, they used (PhS)4Sn as the precursor solution and H2S
as the co-reactant. They found that at 500 �C, uniform
films of SnS were deposited [98]. Juarez et al. [99] de-
posited SnS thin films with the assistance of ‘‘Plasma En-
hanced Chemical Vapor Deposition’’ (PECVD) method.
The electrical and optical characterizations of thin films
based on Sn-S bonds (SnS2, Sn2S3) as a function of the
relative concentration of the precursor vapors, SnCl4 and
H2S were carried out. In all the studied cases, the deposited
films were formed by polycrystalline materials. The au-
thors have reported that SnS2 compound produced under
certain deposition conditions has a forbidden band gap
around 2.2 eV. This compound showed n-type electrical
conductivity with a dark value of 2 9 10-2 (X cm)-1 at
room temperature. Also, it showed the typical semicon-
ductor dependence of its electrical conductivity on the
temperature, with an activation energy of about 0.15 eV.
However, thin films of a mixture of SnS2 and Sn2S3compounds were deposited with higher values of the
relative concentration of vapor sources than those used to
obtain the SnS2 compound. They have also observed that
the optical band gap shows a decreasing trend as the
relative concentration increases. A similar trend was ob-
served for dark electrical conductivity.
3.1.2.4 Dip deposition process Sekhar et al. [141] have
reported the fabrication of SnS and SnS2 thin films. By
means of this technique, a substrate was dipped into an
alcoholic solution of the corresponding tin chloride and
thiourea, then withdrawn vertically at a controlled speed,
and finally baked in a high temperature furnace at atmo-
spheric conditions. Good quality films were obtained at a
baking temperature of 300 and 360 �C. Values of band gap
for SnS and SnS2 obtained from spectral response of
photoconductivity were 1.4 and 2.4 eV, respectively.
Open-air annealing of both SnS and SnS2 films at 400 �Cconverted them into transparent conducting SnO2.
3.1.2.5 Electrodeposition This synthesis route is an
economical method to deposit large area thin films and can
lead to the real mass-production of solar cells. Tin sulfide
thin films were fabricated using conventional three elec-
trode method via constant voltage model. Ichimura et al.
[106, 107] described a three-electrode cell that was used
for ECD with a saturated calomel electrode (SCE) as the
reference electrode. An In2O3 coated glass sheet was used
as the substrate and a stainless sheet as the counter elec-
trode. An aqueous bath used for the deposition contained
SnSO4 and 100 mM of Na2S2O3. SnSO4 concentration [Sn
(II)] was varied between 1 and 7.5 mM. The pH of the
solution was changed in the range between 3.0 and 4.0 by
adding H2SO4 and thin films of SnS were grown at cath-
ode’s surface. The deposition period was 1 h, and the bath
was set to room temperature. Tin sulfide can also be fab-
ricated by constant current Electrodeposition method using
a platinum electrode [112, 142]. SnS films for PV appli-
cation were successfully deposited employing electro-
chemical deposition technique and a detailed report on
electrical characterization results was given by Sato et al.
[26]. On the other hand, SnS thin films deposited over
flexible metallic substrates were studied by Khel et al. [95].
They deposited SnS thin films on Al sheet through this
technique from aqueous solutions containing SnSO4 and
Na2S2O3. The films were polycrystalline with an
orthorhombic structure. Composition was found to be
S-rich in acidic pH and Sn-rich at higher pH values. Re-
lation between film properties and deposition parameters
were also studied in this work to optimize the deposition
conditions. SnS thin films were synthesized by Zainal et al.,
in aqueous media in the presence of Triethanolamine using
this method [110]. Effect of deposition potential, Tri-
ethanolamine concentration, and deposition time on the
properties of SnS films were studied. The presence of
Triethanolamine showed improvement in reproducibility,
adherence and crystallinity of the films. XRD studies
indicated formation of polycrystalline compounds. The
highest photo response was obtained for the film deposited
at -0.80 V in the presence of 0.06 M Triethanolamine.
Films deposited at longer deposition time showed higher
photo response. Absorbance studies revealed that the band
J Mater Sci: Mater Electron
123
gap energy was about 1.20 eV with indirect transitions.
Jain et al. cathodically electrodeposited SnS thin films on
SnO2-coated conducting glass substrates, from an aqueous
solution containing SnCl4 and Na2S2O3 [111]. The films
had Herzbergite orthorhombic crystal structure. Flake/
needle-like crystal structures present in as-deposited sam-
ples were due to the anisotropic growth of various crystal
planes. Interestingly they could observe that annealing of
these needle-like structures resulted in the growth of pla-
telet-like structures. These films were polycrystalline with
an optical band gap of 1.4 eV. Pulse-form electro-deposi-
tion technique was used by Cheng et al. to deposit SnS
films on ITO coated glass substrates [112].
3.1.2.6 Multilayer-based solid-state reaction Tin mono-
sulfide films were synthesized by means of this route by
varying the layer thickness ratios of tin to sulfur; Sn-S films
with different chemical compositions were prepared. The
SnS film with approximate stoichiometric ratio was ob-
tained when the layer thickness ratio of tin to sulfur was set
to 1. The film resulted to be well crystallized with strong
(040) preferential orientation and having a direct band gap
of 1.45 eV. The resistivity and activation energy were
found to be 500 X cm and 0.06 eV, respectively, at room
temperature. In addition, the carrier concentration value
was 2.8 3 1016 cm-3 [119].
3.1.2.7 Spray pyrolysis The spray pyrolysis is a versatile
and economic technique that has been extensively utilized
to synthesize tin monosulfide thin films. In addition, this
route allows an easy way of doping compounds either by
deficiencies in stoichiometry, or by adding an external agent
to the solution with the precursor ion salts. In the year of
1994, Lopez et al. [36] published some results of the SnxSysynthesis by the SP technique. In that work, they reported
that at substrate temperatures of 370–390 �C, the SnS phase
was the predominant phase. Besides, they also determined
its direct band gap energy (1.27 eV) and the activation
energy (0.54 eV). Later, the group of N. K. Reddy et al.
[123] synthesized this compound in the temperature range
of 300–350 �C and calculated an indirect band gap energy
of 1.0 eV. The same group, a year later [124] grown thin
layers of tin monosulfide from equimolar solutions of tin
chloride and N,N-dimethyl thiourea into Corning 7059
glasses. The nozzle presented 2 automatized degrees of
freedom during the deposition (the x–y plane). Single-phase
polycrystalline thin films with a strong preferential orien-
tation along the (111) direction were obtained with a crys-
tallite size of 0.35 lm. Later, Thangaraju et al. [125]
synthesized n-type SnS films at a temperature of 350 �C.The films were highly resistive and amorphous. An indirect
band gap energy of 1 eV was also found for these films. The
films exhibited a photoconductivity character (10 times the
dark conductivity) as well. But, since then, no further re-
ports are available on the application level of these photo-
sensitive films deposited by spray technique. On the other
hand, Ramakrishna et al. [126] deposited SnS single-phase
polycrystalline thin films. All the grown films presented
good adherence to the substrate surface and were pin-hole
free. The layers showed a (111) preferential orientation with
a grain size of 0.35 lm. The films also showed a resistivity
of 30 X cm, a net carrier concentration of 1.2 9 1015 cm-3
and a mobility[180 cm2/Vs with a calculated bandgap of
1.32 eV. Later, these values were corroborated by other
reports. Reddy et al. [127] reported spray pyrolytic depo-
sition of SnxSy films on Sb doped SnO2 glass substrates in
2005. They deposited films at different substrate tem-
peratures and investigated their physical properties. It was
found that films formed in the temperature range of
300–375 �C were nearly stoichiometric with a SnS single
phase and an average grain size of 0.36 lm. The resistivity
of the films was 30 X cm, while the band gap and net carrier
concentration were 1.32 eV and 2 9 1015 cm-3, respec-
tively [127–130].
Moreover, Ramakrishna et al. [63] synthesized and
characterized SnS thin films obtaining similar results to the
previously reported. They also fabricated a heterojunction
solar cell using sprayed SnS as the absorber layer and
indium doped cadmium sulfide as the window layer. Three
years later, Devika’s investigation group [131] explored the
structural behavior of nanocrystalline tin monosulfide
structures with respect to temperature changes. Their
studies also emphasized the dependence of structural
properties of nanocrystalline SnS structures on the sur-
rounding temperature. One year later, Sajeesh et al. [37,
132] reported that the growth temperature sets phase for-
mation: the SnS phase is formed for the growth tem-
perature of 350\Ts\ 400 �C while SnS2 for
Ts[ 400 �C, and Sn2S3 for Ts\ 300 �C. Jeyaprakash
et al. [133] prepared and reported SnS thin films by a home
built microcontroller based spray pyrolysis unit. The X-ray
diffraction analysis confirmed the presence of nanocrys-
talline SnS phase formation with preferential orientation
along (111) plane. By these means, they noticed that a
better crystallinity takes place at higher temperatures. A
direct allowed band gap lying in the range of 1.30–1.40 eV
was noticed with temperature increment. On the other
hand, a study of the photoconductivity and thermoelectric
properties of SnxSy was carried out by Fadavieslam et al.
[134]. Thin films of tin sulfide (SnxSy) with atomic ratios of
y/x = 0.25–1.50 have been prepared on glass substrates at
a temperature of 420 �C. The initial materials for the
preparation of thin films were an alcoholic solution con-
sisting of tin chloride (SnCl4�5H2O) and thiourea
(CS(NH3)2). The SnxSy thin films showed a polycrystalline
structure with a nearly uniform surface and cluster-type
J Mater Sci: Mater Electron
123
growth. By increasing the atomic ratio of (y/x) in films, the
optical band gap, photosensitivity, thermal activation en-
ergy and the Seebeck coefficient changed from 2.72 to
2.37 eV, from 0.05 to 0.78, from 0.07 to 0.48 eV (in the
high temperature range) and from ?0.17 to -0.22 mVK-1
(@ T = 350 K), respectively. In addition, the SnS thin
films structure tends to a nearly single-crystal state in (001)
preferred orientation corresponding to SnS2 phase with
increasing (y/x) ratio. These structure conditions consid-
erably influence the photosensitivity and thermoelectric
properties of thin films.
A broader literature on spray pyrolysis deposition
technique of SnS thin films can be found in the references
[23, 35–38, 63, 125–139].
4 SnS-based thin film solar cell results
Despite the efforts made recent last years in improving
SnS-based solar cells, low efficiency values have been
obtained, with the best value of 4.36 % reached in 2014
[143].
This section is dedicated to a condensed historical re-
view of the works where SnS thin films have been used in
solar cells. Back on 1988, Sharon and Basavaswaran re-
ported a photo conversion efficiency of 0.6 % for a
Photoelectrochemical cell (PEC) with the structure:
n-SnS/Ce4?/Ce3?/Pt. SnS thin films were synthesized by
passing H2S through an solution of SnCl2 [53]. By the
year of 1994, Noguchi et al. [25] successfully deposited
SnS thin films by vacuum evaporation technique and
fabricated an ITO/n-CdS/p-SnS/Ag structure. It exhibited
a short circuit current density (Jsc) of 7 mA/cm2, an open
circuit voltage (VOC) of 0.12 V, a fill factor (FF) of 0.35
and a conversion efficiency (g) of 0.29 %. On the other
hand, a SnS/CdS photovoltaic study was done by Ra-
makrishna et al. [63] in the year 2006 where the SnS
films were synthesized by SP technique and exhibited an
efficiency and quantum efficiency (QE) of 1.3 and 70 %,
respectively. Ghosh et al. [80] fabricated a SnS/CdS
heterojunction by evaporating CdS and SnS films.
A CdCl2-post treatment applied to the window material
presented an increment of grain size. Efficiency values for
solar cells based on window layers with and without
treatment were 0.08 and 0.05 %, respectively, under 1
Sun of intensity. The fabricated cells showed rectification
characteristics. The investigation group of Avellaneda
et al. [144] chemically deposited thin films of SnS in two
different crystalline structures: Orthorhombic SnS (OR)
and Zinc-Blende SnS (ZB). These films showed p-type
conductivity and band gap energies of 1.2 and 1.7 eV,
respectively. A SnO2:F/CdS/SnS(ZB)/SnS(OR) photo-
voltaic structure with an evaporated Ag-electrode was
reported in this paper, exhibiting the following values:
VOC = 370 mV, JSC = 1.23 mA/cm2, FF = 0.44 and
g = 0.2 % under 1 kW/m2 (1 Sun) of illumination. The
methodology on the preparation as well as chemical,
structural and physical characterization results of the Mo/
p-SnS/n-CdS/ZnO heterojunctions were reported by
Bashkirov et al. [71] in 2012. The SnS thin films were
grown by HWVD method on the Mo-coated glass sub-
strates at 270–350 �C. The CdS buffer layers were de-
posited onto the SnS films by chemical bath deposition.
The ZnO window layers were deposited by a two-step rf-
magnetron sputtering method, resulting in a ZnO bilayer
structure: the first layer consists of undoped i-ZnO and the
second of Al-doped n-ZnO. The best junction exhibited
the following parameters: VOC = 132 mV, JSC = 3.6 mA/
cm2, FF = 0.29 and g = 0.5 %. One year later, an opti-
mization of the SnS conduction band offset (CBO) as the
light absorbing layer and Zn1-xMgxO as the buffer layer
in SnS thin film solar cells was carried out to improve the
solar cell conversion efficiency by Ikuno et al. [145]. The
CBO was experimentally controlled by varying the Mg
content of the buffer layer. The optimum CBO value
range for improved solar cell performance was deter-
mined to be from -0.1 to 0 eV. A SnS thin film solar cell
sample with the optimum CBO value exhibited a con-
version efficiency of approximately 2.1 %. Hegde et al.
[74] synthesized SnS polycrystalline thin film by thermal
evaporation (TE) technique in 2013. Electrical resistivity
of the deposited films was about 32.5 X cm with a direct
optical band gap of 1.33 eV. Carrier concentration and
mobility of charge carriers estimated from the Hall
measurements were found to be 6.24 9 1015 cm-3 and
30.7 cm2/Vs, respectively. This research group reported
the fabrication of heterojunction solar cells in superstrate
configuration using TE-SnS as an absorber layer and
CdS:In as window layer. The resistivity of pure CdS thin
film of 320 nm thickness was about 1–2 X cm and was
reduced to 40 9 10-3 X cm upon indium doping. The
solar cells with indium doped CdS window layer showed
improved performance as compared to pure CdS window
layer. The best device had a conversion efficiency of
0.4 % and a fill factor of 33.5 %. A record efficiency was
achieved for SnS-based thin film solar cells by varying
the oxygen-to-sulfur ratio in Zn(O,S) by Prasert et al.
[96]. Studies showed that increasing the sulfur content in
Zn(O,S) raises the conduction band offset between
Zn(O,S) and SnS to an optimum slightly positive value. A
record SnS/Zn(O,S) solar cell with a S/Zn ratio of 0.37
exhibits short circuit current density (Jsc), open circuit
voltage (Voc), and fill factor (FF) of 19.4 mA/cm2,
0.244 V, and 42.97 %, respectively, with an active-area
efficiency of 2.46 %. Recently, this efficiency value was
further improved by adding a SnO2 layer of few
J Mater Sci: Mater Electron
123
nanometers at SnS/Zn(O,S) interface, reaching a new
record efficiency of 4.36 % as reported [143]. A bifacial
SnS solar cell consisting of glass/FTO/SnS/CdS/ZnO/ITO
demonstrated front- and back-side power conversion ef-
ficiencies of 1.2 and 0.2 %, respectively [146]. Low val-
ues for the Jsc during back-side illumination were
exhibited; the diffusion length of minority carrier elec-
trons in the p-type SnS appears to be less than the
thickness of the device because the photogenerated mi-
nority carrier electrons at the back side do not get col-
lected adequately at the SnS/CdS interface to contribute
significantly to Jsc. Both the low back-side Jsc and the
virtual shunt indicate that the Jsc can be increased by
improving charge carrier collection. Two options for im-
proving charge carrier collection include: (1) improving
the minority carrier diffusion length in the SnS bulk by
increasing minority carrier mobility, minority carrier
lifetime or both and (2) using a thinner SnS layer to
reduce charge carrier collection distance necessary. For
the latter, light trapping techniques may be necessary to
maintain adequate light absorption. Nanostructuring the
p-n junction can also reduce the charge carrier collection
distance required. [133].
Some of the solar cell performance parameters of SnS-
based heterojunctions reported by various groups have
been presented in Table 4.
5 Important points to be considered in orderto improve SnS solar cell efficiency
Despite SnS absorber is a potential material for photo-
voltaic applications, solar cells efficiencies based on this
chalcogenide semiconductor are far below those reported
for other absorbers such as CIGS, CdTe, and kesterites. In
order to study if a further solar cell efficiency improvement
is possible, several difficulties that degrade solar cell per-
formance should be highlighted. In general, the following
limiting factors are considered important to improve solar
cell performance:
– Band alignment and density of defect states at SnS/
buffer interface
– SnS bulk defects and secondary phases formation
– Short minority carrier lifetime and diffusion length
– SnS-back contact and solar cell configuration
Table 4 Photovoltaic properties of tin monosulfide thin film solar cells
Cell VOC
(mV)
JSC(mA/cm2)
FF
(%)
g(%)
RS
(kX cm2)
RSH
(kX cm2)
n J0 9 10-7
(mA/cm2)
Year References
p-SnS/Fe3? 320 0.65 65 0.54 – 2.5 – – 2001 [147]
SnS/CdS 260 9.6 53 1.3 0.023 – – – 2006 [63]
SnS/CdS 274 0.31 40 0.08 0.505 2.14 1.83 – 2008 [80]
ZnO/SnS 120 0.04 33 0.003 5.57 1.64 1.28 1.0 2009 [148]
SnS(OR)/SnS(ZB)/CdS 370 1.23 44 0.2 0.5 18 – 5 2009 [149]
SnS/TiO2 471 0.3 71 0.1 0.27 0.0349 – – 2010 [150]
SnS/CdS 183 2.7 34 0.17 – – – – 2011 [151]
p-SnS/n-SnS 280 9.1 29.9 0.74 – – – – 2012 [152]
Mo/SnS(CVD)/CdS/ZnO 132 3.63 29 0.5 0.04 0.35 4 0.2 2012 [71]
Zn0.83Mg0.17O/SnS 270 12.1 64 2.1 – – – – 2013 [145]
CdS/SnS 208 17.9 38 1.6 0.005 0.0312 – – 2013 [153]
SnS/CdS:In 302 3.98 33.5 0.4 0.169 0.503 – – 2013 [74]
SnS/Zn(O,S) 220 16.8 47.7 1.8 – – – – 2013 [96]
244 19.42 42.97 2.04 – – – –
TCO/CdS(0.3 llm)/
SnS(1.8 llm)/C/Ag
270 6 44 0.7 – – – – 2014 [144]
Mo/SnS/Zn(O,S)/ZnO/ITO 261 24.9 44.4 2.9 – – – – 2014 [154]
Glass/FTO/SnS/CdS/ZnO/ITO
Front side 200 15 40 1.2 – – – – 2014 [146]
Back side 140 1.3 34 0.2 – – – –
Mo/SnS/SnO2/Zn(O,S)/ZnO/ITO 372 20 58 4.36 – – – – 2014 [143]
J Mater Sci: Mater Electron
123
5.1 Band alignment and density of defect states
at SnS/buffer interface
One of themost important issues in SnS solar cells is low open
circuit voltage. In fact, for the best solar cell efficiency re-
ported up to date (4.36 %), an open circuit voltage value of
372 mVusing Zn(O,S) as buffer layer is reported [143]. Band
alignment at SnS/buffer is commonly assumed to be the main
hurdle that produces low open circuit voltage values.
To find one adequate buffer material could be one of the
greatest challenges for SnS technology. In order to overcome
that problem, someworks have been focused onfinding a better
buffer candidate. For that purpose, band alignment studies have
been reported for CdS [155, 156], SnO2 [155], ZnMgO [157],
and Zn(O,S) [158]. Among them, Zn(O,S) showed a better
alignment with SnS. In particular, for S/Zn ratios lower than
0.5, small positive conduction band offsets (spike-like) as
shown in Fig. 1a were reached. From a theoretical point of
view, a small CBO in the range of 0 eV to 0.4 eV is the optimal
band alignment [159, 160]. Outside this range, a negative CBO
(cliff-like), as shown in Fig. 1b, suffers from increasing inter-
face recombination, while a large positive CBO forms a barrier
that reduces photocurrent collection. Despite Zn(O,S) align-
ment was better, no significant improvements in solar cell ef-
ficiency have been reached. Therefore, lowopen circuit voltage
could be related to other aspects such as defects at SnS/buffer
interface, bulk defects, etc. If there is a significant lattice mis-
match between the two component materials, a high interfacial
defect density at SnS/buffer interface could characterize SnS/
buffer junction reducing open circuit voltage value. So far,
there is no report about defect states study at SnS/buffer junc-
tion and its effect on solar cell performance. Such study could
help to clarify Voc losses.
5.2 SnS bulk defects and secondary phases
formation
The low performance could also be blamed on poor film
quality, i.e., polycrystalline films with the presence of
multiple secondary phases. Diode quality factors for SnS
devices are reported in the range of 1.83–1.92, [63],
indicating substantial recombination in the space charge
region (SCR). Short-circuit current collection in SnS de-
vices is on par with that achieved in kesterite devices [1],
which along with the high diode quality factor (*2) is
consistent with losses primarily due to recombination.
These losses are mainly related to interface defects and/or
bulk states which highly depend on deposition technique.
Therefore, an improvement in crystalline quality is re-
quired to improve solar cell output. Furthermore, further
studies are also needed in order to elucidate the influence
of both interface and bulk defects and which of them has
a major impact on the Voc value. On the other hand, at
least two secondary phases could be formed along with
SnS compound (Sn2S3, and SnS2). Despite secondary
phases have shown an important role in kesterite com-
pounds [1], the recent application of atomic layer and
chemical vapor deposition (ALD/CVD) techniques has
succeeded in producing high-quality phase pure films [65,
161] without a significant increase in efficiency. There-
fore, secondary phases could have a low impact on solar
cell performance. As a result, future progress in SnS solar
cells should be rely on understanding the defects that
lower Voc and the nature of defects near the SnS/buffer
heterojunction.
5.3 Short minority carrier lifetime and diffusion
length
SnS compounds are characterized by low minority carrier
diffusion length values (0.18–0.23 lm) [162]. This implies
low lifetime and mobility values. Low minority carrier
diffusion length values determine low values of Voc. Im-
proving the morphological properties and the crystalline
quality of the films involved in the solar cells will guar-
antee an improvement in the charge carrier transport
parameters.
Fig. 1 Band alignment for SnS/
buffer heterojunction: a spike-
like configuration and b cliff-
like configuration
J Mater Sci: Mater Electron
123
5.4 SnS back contact and solar cell configuration
The majority of SnS solar cells produced to date have been
based on adopting the architecture developed for CIGS,
where the absorber (SnS) is deposited on Mo-coated glass
as displayed in Fig. 2a. However, this metal could de-
compose SnS compound to form secondary phases in the
back contact such as MoS2 which can behaves as a
blocking back contact. A similar problem is presented in
kesterite compound which solar cell configuration is
mostly based on Mo as back contact [1]. This could explain
the complex temperature dependence observed for SnS
Ohmic contacts [163]. Therefore, the option of using other
types of metals is an open problem.
On the other hand, most solar cells reported have been
fabricated with the structure of substrate or CdS/CIGS
(Fig. 2a). The option of fabricating devices in a superstrate
structure, i.e. the deposition of buffer onto TCO, followed
by the deposition of the absorber film as shown in Fig. 2b,
could favor the properties of the solar cells, especially
when deposition methods of absorber imply high roughness
of the films such as spray pyrolysis. In this way, the
roughness should have less impact in the properties of the
solar cells.
It is also important to mention that a Metal–Insulator-
Semiconductor (MIS) behavior has been observed in CdTe
and kesterite Cu2ZnSnSe4 compounds and results have
been published [164–166]. This performance is due to the
buffer layer can be considered as an insulator between the
TCO that behaves like a metal and the p-type semicon-
ductor. As a result of this character, an improvement in Voc
values has been observed when CdS is doped with Cu,
which implies an increase in buffer layer resistivity value.
In other words, better solar cell efficiencies have been
obtained for thinner and resistive buffer layers. If SnS solar
cells behave as a MIS structure, a Voc enhancement should
be reached by increasing buffer resistivity, but further
studies are needed to demonstrate that performance. This
could help to improve one of the most important limiting
parameters in SnS-based technology.
In summary, in addition to high-quality material, SnS
cells must have optimized window and back-contact in-
terfaces to minimize recombination, resistive losses, and
parasitic absorption. While the present Zn(O,S) buffer may
be adequate to address some of the most urgent absorber
development needs, moving to higher band-gaps and im-
proved light transmission will require buffer development
similar to that being carried out for CIGS devices. In ad-
dition to determining and optimizing the interfacial band
offset, understanding band bending, interfacial defect
concentration, inter-diffusion and stability among other
properties is necessary to minimize recombination.
6 Conclusions
In this work, we present a review about the state of the art of
SnS films and devices along with the analysis about different
factors that are limiting solar cell performance. In summary,
there are several issues that must be understood in order to
overcome present limits in Voc values. In order to reach a
further improvement in SnS solar cell efficiency, it is re-
quired to obtain high-quality SnS material. Besides, some
other important aspects such as recombination at SnS/buffer
interface and bulk materials must be improved. On the other
hand, to find an adequate back-contact for replacing Mo,
could improve solar cell performance. Furthermore, in ad-
dition to determining and optimizing the interfacial band
offset, understanding band bending, interfacial defect con-
centration, inter-diffusion and stability among other prop-
erties is necessary to minimize recombination.
Acknowledgments This work was partially supported by CeMIE-
Sol-207450/P26. J.A. Andrade-Arvizu thanks Raul Andrade & Car-
men Arvizu for everything. J.A. Andrade-Arvizu and M. Courel thank
Conacyt and BEIFI fellowship supports. O. Vigil-Galan acknowl-
edges support from COFAA and EDI of IPN.
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