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Liquid Phase Exfoliated Indium Selenide Based Highly
Sensitive Photodetectors
Nicola Curreli, Michele Serri, Davide Spirito, Emanuele Lago, Elisa Petroni,
Beatriz Martín-García, Antonio Politano, Bekir Gürbulak, Songül Duman,
Roman Krahne, Vittorio Pellegrini, and Francesco Bonaccorso*
Layered semiconductors of the IIIA–VIA group have attracted considerable
attention in (opto)electronic applications thanks to their atomically thin
structures and their thickness-dependent optical and electronic properties,
which promise ultrafast response and high sensitivity. In particular, 2D
indium selenide (InSe) has emerged as a promising candidate for the
realization of thin-film field effect transistors and phototransistors due to its
high intrinsic mobility (>102 cm2 V−1 s−1) and the direct optical transitions in
an energy range suitable for visible and near-infrared light detection. A key
requirement for the exploitation of large-scale (opto)electronic applications
relies on the development of low-cost and industrially relevant 2D material
production processes, such as liquid phase exfoliation, combined with
the availability of high-throughput device fabrication methods. Here, a β
polymorph of indium selenide (β-InSe) is exfoliated in isopropanol and
spray-coated InSe-based photodetectors are demonstrated, exhibiting
high responsivity to visible light (maximum value of 274 A W−1 under
blue excitation 455 nm) and fast response time (15 ms). The devices
show a gate-dependent conduction with an n-channel transistor behavior.
Overall, this study establishes that liquid phase exfoliated β-InSe is a valid
candidate for printed high-performance photodetectors, which is critical
for the development of industrial-scale 2D material-based optoelectronic
devices.
N. Curreli, Dr. M. Serri, Dr. E. Lago,[++] E. Petroni,[++] Dr. B. Martín-García,
Dr. A. Politano,[+++] Dr. V. Pellegrini, Dr. F. Bonaccorso
Graphene Labs
Istituto Italiano di Tecnologia
via Morego 30, 16163 Genova, Italy
E-mail: francesco.bonaccorso@iit.it
N. Curreli
Dipartimento di Ingegneria Elettrica ed Elettronica
Università di Cagliari
P.zza d’Armi, 09123 Cagliari, Italy
The ORCID identification number(s) for the author(s) of this article
can be found under https://doi.org/10.1002/adfm.201908427.
[+]Present
address: IHP—Leibniz-Institut für innovative Mikroelektronik,
Im Technologiepark 25, 15236 Frankfurt (Oder), Germany
[++]
Present address: STMicroelectronics, SMART POWER Technology
R&D, Via C. Olivetti 2, 20864 Agrate Brianza, Italy
[+++]Present address: Dipartimento di Scienze Fisiche e Chimiche,
Università degli Studi dell'Aquila, Via Vetoio, 42, 67100 Coppito, Italy
DOI: 10.1002/adfm.201908427
Adv. Funct. Mater. 2020, 30, 1908427
1. Introduction
2D semiconductor materials, including
layered transition metal dichalcogenides
(TMDs) with formula MX2 (M = Mo, W;
X = S, Se, Te), have been intensely studied
as substitutes for conventional semiconductors in opto-electronic applications.[1,2]
The β polymorph of indium selenide
(β-InSe) is a promising van der Waals
layered material due to its remarkable
fundamental properties,[3] such as a low
electron effective mass (m* = 0.143 m0)[4]
and a bandgap ranging from ≈1.26 eV
for the bulk to ≈2.11 eV for the monolayer at room temperature,[5,6] crossing
over from an indirect to a direct semiconductor when the crystal thickness is
larger than six layers (≈5 nm, each layer
is ≈0.84 nm thick).[7–9] The fundamental
properties of β-InSe indicate the potential use of few-layer flakes in field effect
transistors (FETs) and sensitive electric
light detectors thanks to a direct bandgap,
which is tunable by the crystal thickness
in a wide spectral range from visible to
Dr. D. Spirito,[+] Dr. R. Krahne
Nanochemistry Department
Istituto Italiano di Tecnologia
Via Morego 30 ,16163 Genova, Italy
Dr. E. Lago, E. Petroni
Dipartimento di Chimica e Chimica Industriale
Università degli Studi di Genova
via Dodecaneso 31, 16146 Genoa, Italy
Dr. B. Gürbulak
Department of Physics
Faculty of Sciences
Atatürk University
25240 Erzurum, Turkey
Prof. S. Duman
Department of Basic Sciences
Faculty of Sciences
Erzurum Technical University
25050 Erzurum, Turkey
Dr. V. Pellegrini, Dr. F. Bonaccorso
BeDimensional Spa
via Albisola 121, 16163 Genova, Italy
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near-infrared (NIR) light.[5,10] Several groups reported n-type
FET based on single layer and thin InSe crystals with values
of electron mobility of µe ≈ 103 cm2 V−1 s−1.[11,12] Photodetectors with a photoresponsivity Rph ≈ 5 × 107 AW−1 in single flake
devices,[8,13–18] surpassing TMDs[19,20] and rivalling other high
mobility (≥102 cm2 V−1 s−1) direct bandgap 2D semiconductors
such as black phosphorus (BP)[21,22] have also been demonstrated. Furthermore, a lower enthalpy of oxygen chemisorption on monolayers of InSe compared to single layer BP makes
it more environmentally stable compared to the latter.[23]
The high responsivity of β-InSe photodetectors has been
explained by the direct bandgap of thick (>5nm) flakes, which
results in efficient light absorption in the material.[24] Extrinsic
factors due to the photodetector design (e.g., short channel
length) may raise the responsivity as well.[18,25] Moreover, the
presence of photoconductive gain mechanisms in β-InSe also
contributes to the high responsivity, multiplying the number
of electrons flowing in the device per absorbed photon.[26] In
particular, the presence of traps that reduce the mobility of
minority carriers (holes) in the material, results in the circulation of photogenerated electrons multiple times through the
device before recombination.[19] Unfortunately, the increased
responsivity gain comes at the expense of a slower response
time of the photodetector,[27] which might be problematic for
applications that require a high bandwidth, such as imaging[28]
or optical communication.[29] Furthermore, trap-assisted recombination results in sublinear dependence of the responsivity
as a function of the light intensity, limiting the sensitivity at
high optical power and complicating the readout of the photodetector signal.[30] Therefore, the study of the charge trapping
and recombination mechanisms in InSe could provide insights
for the optimization of the semiconducting material and the
device design for different application requirements.
Although promising figures of merit, FoM, (µe, Rph)
have been reported for InSe devices, the aforementioned
results were obtained using single-flake devices, produced by
low-throughput methods of fabrication, such as mechanical
exfoliation[14] of bulk crystals followed by manual assembly[31] of
heterostructures. The latter requires the identification of suitable flakes and a precise alignment of the electrodes by electron
beam lithography (EBL).[18] Thus, to enable the adoption of this
material in consumer electronics, scalable and sustainable processes for both material production and device fabrication are
needed. To this end we recall that chemical vapor deposition
of InSe films with mostly monolayer thickness was achieved
recently over areas of 1 cm2, enabling the fabrication of n-type
FETs with electron mobility up to ≈30 cm2 V−1 s−1.[32–34] Wafer
scale growth of InSe films by pulsed laser deposition has also
been demonstrated, producing films with an electron mobility
of 10 cm2 V−1 s−1 and a response of 27 A W−1 in phototransistor
devices.[35] These techniques require a fine tuning of the growth
parameters (e.g., temperature, growth duration),[36] expensive
equipment,[37] and high temperature (>600 °C)[32,35] conditions,
which increase the energy requirements for the device fabrication. Therefore, they still do not represent the solution for
consumer electronics application.
Liquid phase exfoliation (LPE)[38–40] is another process that
was successfully exploited to produce few layer InSe crystals,
offering advantages over the aforementioned methods in terms
Adv. Funct. Mater. 2020, 30, 1908427
of costs and scalability.[41] Although, the compatibility of the
inks with high-throughput printing processes and the level of
performance of InSe printed devices still needs to be assessed,
LPE might represent a viable approach to exploit InSe fewlayers for optoelectronic applications.
We remark that LPE allows the exfoliation of layered
materials in a liquid medium in ambient conditions,[42]
applying an external stimulus such as ultra-sonication,[42,43]
high-shear mixing,[44,45] ball milling,[46,47] wet jet milling,[48]
and microfluidization.[49] For the efficient exfoliation of layered
materials, the solvent should prevent restacking and aggregation of the exfoliated layers by satisfying specific surface energy
requirements for the considered material, which are summarized by the solvent surface tension and the Hansen solubility
parameters.[50,51] Usually, the dispersions produced by LPE
have a heterogeneous composition of exfoliated flakes both
in lateral size and thickness,[43] which can be fractioned, for
example, by using sedimentation based separation (SBS).[52–55]
The as-produced flakes are mostly basal plane defect-free and
unfunctionalized.[41,43,53–55] In addition, LPE is the ideal tool for
the formulation of inks[50,53,56] and pastes,[57,58] as well as for the
integration of the exfoliated flakes in composites,[59] and coatings.[60,61] This makes dispersions of 2D materials appealing for
the realization of fully printed devices.[50,53,56]
From the production point of view, the choice of the solvent is a critical issue of the LPE process. In fact, common
solvents used for the formulation of 2D material based inks (e.g.,
N-methyl-2-pyrrolidone—NMP,
dimethylformamide—DMF,
N-cyclohexyl-2-pyrrolidone—CHP), present serious health hazards (e.g., NMP, DMF, CHP, health code ≥ 2 NFPA704).[62] Furthermore, the low vapor pressure (Pv ≈ 0.05 kPa)[63] and high
boiling point (Tb ≈ 200 °C)[64] of the aforementioned solvents
result in surface contamination of the exfoliated flakes with an
insulating organic layer, which is detrimental for the electronic
conduction of the exfoliated materials.[18,65,66] Recently, LPE of
2D materials in low boiling point solvents such as acetone,[67]
alcohols,[50] and water/alcohol co-solvent systems[18,50,68–70] has
been investigated as a strategy to reduce the use of toxic chemicals, minimizing the contamination by solvent residuals in
films of LPE flakes.
The LPE exfoliation of InSe has been achieved by ultra-sonication by using isopropyl alcohol (IPA)[69] and water-ethanol
(H2O/EtOH) mixtures,[18] allowing an effective removal of the
solvent by heating at moderate temperatures (e.g., ≈50 °C)
thanks to their low boiling point (78.2 °C < Tb < 100 °C).[62] In
particular, the Hersam’s group demonstrated that InSe flakes
(average thickness of 41 nm) exfoliated by ultra-sonication in
deoxygenated H2O/EtOH mixtures exhibit electron mobilities
µe ≈ 19 cm2 V−1 s−1 and photoresponsivity Rph ≈ 5 × 107 A W−1
in single flake phototransistors.[18] On the other hand, devices
produced with InSe flakes exfoliated in high boiling point
solvents (i.e., NMP, DMF) have shown lower performance,
compared with the one produced in H2O/EtOH mixtures,
due to organic contaminants.[18] The same study reported a
responsivity of Rph = 10 AW−1 in devices fabricated from InSe
based films obtained by membrane filtration of the dispersions in H2O/EtOH, which resulted in percolating networks of
flakes manifesting a deterioration of the photodetector performance compared to the single flake.[18] This phenomenon is a
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consequence of the high contact resistance between flakes compared to the intrinsic resistance of the flakes themselves and
is exacerbated in the case of percolating films due to electrical
conduction occurring through an increased number of interflake boundaries. Although these results highlight the potential
of LPE InSe based optoelectronics from a fundamental point of
view, the feasibility of scalable and repeatable processes used in
industrial production has not yet been investigated.
In this work, we produce β-InSe inks by ultrasound-assisted
LPE in IPA and use spray coating deposition of the inks on
silicon substrates to fabricate highly responsive photodetectors.
Spray coating is an industrially compatible process that can be
optimized to produce highly uniform films of electronically
active materials and has already been applied to the fabrication
of perovskite based solar cells.[71,72] Our results show that the
photodetectors exhibit high responsivities to light in a broad
spectral range (450–900 nm), with a maximum responsivity
Rph = 274 AW−1 at 0.53 mW cm−2 irradiance and a rise time
of ≈15 ms. Our photodetector outperforms, in term of responsivity, previous devices based on percolating networks of solution processed 2D flakes[18] by more than one order of magnitude. By studying the optical power dependence of the responsivity and the time-dependent profiles of the photocurrent
under light modulation, we conclude that the recombination
rate of the photocarriers is a cubic function of the concentration
of charge carrier density. We suggest that the third order rate
dependence could be related to a recombination mechanism
assisted by doubly charged Se vacancies.
2. Results and Discussion
2.1. Material Production and Characterization
The synthesis of β-InSe monocrystals was performed with
the Bridgman–Stockbarger method.[73] InSe can exist in three
crystal polymorphs, β, γ, and ε, that differ only in the layers
stacking.[3,74,75] The crystal structure obtained by this method
has the β form, as determined by X-ray diffraction (XRD).[73]
Based on the study of the LPE of β-InSe in IPA reported by
Petroni et al.,[69] we performed sonication and ultracentrifugation (see Section 4) in order to achieve a good compromise
between ink stability, the lateral size, and thickness of the
flakes. The concentration of the exfoliated β-InSe flakes was
evaluated by means of optical extinction measurements. The
concentration of the obtained dispersion is 0.11 g L−1, as estimated by the Beer–Lambert law
αc =
A
l
(1)
A
is the absorbance per length, c is the concentration
l
and α is the extinction coefficient with α ≈ 580 L g−1 m−1 at
600 nm.[69] As reported in ref. [69], a typical extinction spectrum of the β-InSe dispersion (Figure S4, Supporting Information) exhibits features at ≈275 nm and at ≈360 nm, which
correspond to direct electronic transitions between valence
and conduction band.[76] In order to confirm the production of
where
Adv. Funct. Mater. 2020, 30, 1908427
few layer β-InSe flakes with no defects, the efficacy of the exfoliation of the crystal was evaluated by morphological, chemical,
and structural analyses. Raman spectroscopy measurements,
shown in Figure 1a, were performed in order to demonstrate
the absence of other chemical species, (e.g., In2Se3, In2O3)[75,77]
that could have been formed during the exfoliation process or
subsequent exposure to atmosphere. β-InSe has six Raman
active vibrational modes, which are assigned to the peaks in the
spectra in Figure 1a[74,77] in both the bulk and exfoliated β-InSe
samples. The data confirms the absence of polymorph crystals.
Peaks related to other In and Se compounds or oxidized phases
are not present, suggesting that the exfoliated flakes keep their
crystalline integrity.[75,77] These conclusions are also supported by
X-ray photoelectron spectroscopy (XPS) spectra of the In 3d and
Se 3d regions (Figure S5, Supporting Information), showing only
a 0.2 eV broadening of the peaks in the exfoliated material, which
is indicative of a slight increase in defects and oxide species compared to the bulk, and the XRD patterns shown in Figure 1b.
These data are in agreement with the diffraction of β-InSe
(ICDD 98-018-5172). The XRD patterns demonstrate, both for
bulk and for exfoliated samples, the occurrence of a hexagonal
β-InSe structure with lattice parameters of a = b = 4.005 ± 0.004 Å
and c = 16.660 ± 0.004 Å.[69] Moreover, the β-InSe bulk crystals
exhibit only reflections belonging to the (001) family, indicating
strong texture of crystalline flakes along the c axis. In the exfoliated β-InSe flakes, we notice also reflections from other orientations (e.g., 010, 110, and 011), due to disordered arrangement
of the nanocrystals, although a strong preferential orientation
of the (001) plane is still present. Figure 1c,d reports representative transmission electron microscopy (TEM) and atomic
force microscopy (AFM) images of the exfoliated β-InSe flakes,
respectively. Statistical analysis using a log-normal distribution[78]
(Figure 1e) indicates that the exfoliated β-InSe flakes have a typical
lateral dimension (mode) of ≈113 nm (σ = 0.84), corresponding
to an average surface area of ≈6.1 × 10−3 µm2, and a thickness
of ≈4 nm (σ = 0.54) as measured by AFM in Figure 1f. Therefore, based on the thickness of monolayer β-InSe (≈0.9 nm),[79,80]
flakes with single/few layers are effectively produced.
2.2. Phototransistor Fabrication and Characterization
We investigated the application of β-InSe based inks in printed
photodetectors using a spray coating deposition method. The
inks exhibit low viscosity (η25° ≈ 3.2 mPa × s at 25 °C), with
Newtonian behavior at shear rates between 0.2 and 300 s−1
(Figure S1, Supporting Information), which makes them suitable for spray coating deposition.[81] An interdigitated gold
electrode array was fabricated using EBL and lift-off (see
Section 4) on highly p-doped (boron) silicon (100) with 100 nm
thermal oxide (SiO2) on the surface. The interdigitated design
allows to achieve a low electrical resistivity, by reducing the
gap between electrodes L and increasing the total width of the
conduction channel W, in a more compact format compared to
linear electrodes, by using a parallel array of finger electrodes.
Additionally, the reduction of L leads to a faster response of the
photodetector[82] by reducing the transit time of the carriers.
The electrodes used in our devices consist of 65 interdigitated
fingers with an overlap of 40 µm and a gap L = 1 µm, which
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Figure 1. Morphological, chemical, and structural characterization of β-InSe flakes. a) Raman spectra for bulk β-InSe (blue trace) and exfoliated β-InSe
(red trace) samples. b) XRD diffractogram for bulk β-InSe (blue trace) and exfoliated β-InSe (red trace) samples. c) Representative TEM image of an
isolated β-InSe flake. d) Representative AFM image of an isolated β-InSe flake. Height profile (solid white line) of the indicated section (white dashed
line) is also shown. e) Lateral size statistical analysis for β-InSe flake dispersion. f) Statistical analysis of the thickness of β-InSe flakes in the dispersion.
results in an overall channel width W = 5160 µm, providing
an active area of W × L = 5760 µm2 for photodetection. During
the same lithographic process, several Au electrode arrays were
Adv. Funct. Mater. 2020, 30, 1908427
deposited by e-beam evaporation on the same substrate to
exploit the large area deposition capability of the spray coating
process. A volume of ≈30 mL of the as-produced β-InSe ink in
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Figure 2. a) Schematic illustration of the β-InSe photodetector. b) Optical microscope image of the complete photodetector and c) magnified detail
of the conducting channel region. d) SEM image of the β-InSe film in the conducting channel region of the device. e) Dark source–drain current (ID)
versus source–drain voltage (VD), at bottom gate voltages between −40 and 40 V. In the inset, a log–log plot of ID versus VD (VG = 0 V) is depicted,
showing the transition from ohmic to space charge limited conduction. f) Source–drain current (ID) versus gate voltage (VG) curve at VD = 2 V, obtained
from the data in (e).
IPA was deposited by spray-coating onto the patterned substrate,
which was heated to 60 °C to favor film drying during the deposition process. The coated sample was placed under vacuum
overnight at room temperature and then annealed at 200 °C
for 30 min in argon atmosphere to stabilize the deposited film
and remove residues of adsorbed solvent and moisture. The
film thickness was 515 ± 107 nm, as measured by profilometry
(Figure S2, Supporting Information). The basic structure of the
β-InSe photodetector is illustrated by the scheme in Figure 2a
and optical microscope images in Figure 2b,c.
Figure 2d shows the top-view scanning electron microscopy (SEM) image of the β-InSe film deposited on the electrodes, presenting a percolating network of flakes of lateral size
<500 nm. Energy-dispersive X-ray (EDX) spectroscopy (Figure S3,
Supporting Information) was performed during SEM imaging,
confirming the presence of β-InSe flakes in the film. From the
EDX analysis on the device, we determined a ratio of 1:0.87
between In and Se, in agreement with previous characterization of the exfoliated β-InSe performed by our group.[69] The
elemental composition, within the experimental uncertainty of
EDX, indicates the presence of selenium vacancies in the semiconductor film.[69] The signal from oxygen can be explained
mostly by the SiO2 layer on the surface of the substrate,
although a superficial oxidation of the β-InSe flakes is also
possible due to the processing in air.
The current–voltage (ID–VD) curves of the β-InSe photodetector were measured at room temperature and under vacuum
Adv. Funct. Mater. 2020, 30, 1908427
to avoid the influence of moisture and atmospheric gases. The
doped silicon substrate was electrically contacted to apply a gate
bias VG. As shown in Figure 2e, the drain-source current (ID)
varies with drain voltage VD under different VG (from −40 to
40 V) in dark condition, displaying a gate-tuneable behavior,
indicating that the electrical characteristics of β-InSe device can
be effectively controlled by electrostatic doping. In the inset to
Figure 2e, a quasi-linear regime (slope of the curve r = 1.2) for
0 < VD < 0.5 V suggests ohmic contacts between the gold electrode and β-InSe. At larger bias with 0.5 < VD < 2 V, a quadratic dependence of the drain current is observed, which can be
explained by a space-charge limited current (SCLC) regime.[83]
SCLC becomes dominant when the injected electron concentration exceeds that of the thermally generated one. Charge-carrier
traps within the semiconducting film, located, for example,
in the partially oxidized surface of the flakes, are effective in
immobilizing most of the injected electrons.[84,85] For shallow
traps located at an energy Et below the conduction band edge,
the SCLC current density is given by a quadratic relation with
respect to the voltage (I D ∝ VD2).[83] Figure 2f shows the ID–VG
transfer curves in the dark at a drain bias voltage of 2 V. The
device exhibits an ambipolar behavior with a minimum ID current at VG ≈ −10 V and a distinct asymmetry in electron and hole
conduction, showing an average mobility of the film (defined in
the linear regions of the ID–VG curve) of 3 × 10−5 cm2 V−1 s−1
for the electrons and 1 × 10−5 cm2 V−1 s−1 for the holes. We
attribute the decrease in mobility compared to single flake
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Figure 3. a) Photocurrent response for varying incident light power on the active area of the device measured at three different wavelengths. The
dashed lines represent a power-law fit to the data. The inset plots the photoresponsivity Rph versus the irradiance Ir. b) Spectral responsivity of β-InSe
photodetector. The dashed line is a linear fit of the tail of the spectrum; the onset of the photoresponse at ≈900 nm (1.38 eV) is highlighted. The inset
plots the response to 0.1 Hz pulsed light (530 nm) c) Detail of photocurrent rise and decay during pulsed (2 Hz) 625 nm light excitation. d) Plot of
the time derivative of the photocurrent versus the photocurrent after switching off the light. Inset: Responsivity versus light chopping frequency under
illumination at 625 nm. Dashed lines indicate the power laws f−0.5 and f−0.2.
values to the presence of traps and the surface oxidation during
spray deposition processing in air, which increases the contact resistance between the flakes.[86] The transistor is n-doped
at VG = 0 V and, for this reason, no off-state condition can be
measured. This phenomenon could be explained by the presence of the defect states in the gap of β-InSe. The n-doping
in InSe nanoflakes was also confirmed by the position of the
Fermi level compared to the valence and conduction bands,
as determined through ultraviolet photoelectron spectroscopy
(UPS) (Figure S6, Supporting Information).
In order to reveal the photodetection behavior of the device,
the electrical characteristics were measured under the exposure
to light of different wavelength and intensity. The photodetector
response is measured as photocurrent (Iph), corresponding
to the difference between the current measured (at VD = 2 V,
VG = 0 V) under light and in the dark, for light intensities (Ir)
between 0.5 and 7.5 mW cm−2. Figure 3a reports the photocurrent as a function of the light power on the device, using
three different LEDs with emission peaks at 455, 530, and
625 nm (FWHM = 17, 42, 20 nm, respectively). The dependence on light power is sublinear; therefore, the photoresponsivity (Rph, inset of Figure 3a), defined as
R ph =
I ph
Ir ⋅ S
Adv. Funct. Mater. 2020, 30, 1908427
(2)
(in which Ir is the irradiance, S is the active area of the device),
is decreasing as the power increases. The maximum measured
responsivity at 455 nm is ≈274 AW−1, at ≈0.53 mW cm−2 irradiance. The device maintained its functionality even in ambient
conditions and after 1 year (Figure S7, Supporting Information). To assess the minimum detectable light intensity, we
calculated the detectivity, defined as[87]
D* =
S
NEP
(3)
Si
is the noise equivalent power and Si is
Rph
the spectral density of the noise current. We obtained a maximum value (corresponding to the maximum responsivity) of
NEP ≈1.31 × 10−15 W Hz−0.5 and D* ≈ 5.49 × 1012 Jones. These
values are obtained estimating Si by the sum of two noise
mechanisms: the thermal noise Sc = (4kT/Rdark)0.5, calculated
considering the dark resistance Rdark of the device, and the shot
noise, Ss = (2eIdark)0.5, from the dark current Idark.
These FoM values compare favorably with those reported in
literature.[88–91] The responsivity is at least one order of magnitude higher than those of photodetectors based on solution
processed 2D crystals, and InSe in particular.[18] There are
several factors that can cause the increased responsivity of
our device. The short length of the channel (L) increases the
In which NEP =
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photoresponsivity of the device, since Rph is proportional to
L−2.[25] Moreover, the highly uniform coverage of β-InSe on
the Si/SiO2 substrate over the active area could promote the
extraction efficiency of the photogenerated carriers as already
suggested in literature for perovskite-,[92] thin-film CdTe[93] and
graphene based devices.[94]
The spectral response of the device is shown in Figure 3b
from the visible to the NIR range, measured with mechanically
chopped light at 23 Hz (see Section 4) at bias voltages VD = 2 V
and gate voltage VG = 0 V. The responsivity is high at short wavelength (≈400 nm) and decreases towards longer wavelength with
a pronounced drop at ≈800 nm. If the wavelength dependence
is dominated by the absorption coefficient, it is possible to estimate the bandgap from the intercept with the wavelength axis
of a linear fit of the spectral responsivity in the region near the
photoresponse threshold wavelength (Figure 3b). The resulting
value of ≈900 ± 65 nm corresponds to a bandgap of ≈1.4 ± 0.1 eV,
which is in the range between the values reported for single
layer and bulk β-InSe (2.11–1.26 eV respectively), confirming
that the film is composed by few layer flakes. These results are
also supported by the observation of a broad photoluminescence
(PL) peak at 959 ± 50 nm (Figure S8, Supporting Information).
Finally, in Figures 3b (inset) and 3c we report the time response
of the device, obtained by measuring the current during pulsed
light excitation. Excellent long-term stability is observed with a
fast switching and reproducible transition from “ON” to “OFF”
conditions. The measured rise (fall) time (Figure 3c), defined
as the time to pass from 10% (90%) to 90% (10%) of the maximum photocurrent, is τR = 15.1 ms (τF = 63.7 ms), while other
photodetectors made with films of LPE flakes of β-InSe reported
response times of the order of seconds.[10,18] In the inset to
Figure 3d, we report the dependence of the photocurrent amplitude on the modulation frequency f. The amplitude decreases
with the increase of the frequency, and the signal is measurable
up to 1 kHz; the functional dependence of the frequency does
not follow a simple low-pass behavior but exhibits richer features with complex power-law trends that follow a f−0.5 and f−0.2
dependence at low and high modulation frequency respectively,
as shown by dashed lines in the panel. Such behavior could indicate an energy distribution of trap states in the material.
The time decay of photocurrent in Figure 3c can be investigated more in detail to understand the mechanism of charge
recombination in our device. In general, the time derivative of
the photoexcited charge density n, after turning off the light, is
a function of n itself.
dn
= g (n )
dt
(4)
Assuming that the photocurrent is proportional to n, the
function g can be determined from the time dependence of Iph
during the decay measurement. In Figure 3d we plot the photocurrent derivative (dIph(t)/dt) versus Iph after light was switched
off. A third-order polynomial yields an excellent fit to the data
(dashed line in Figure 3d), suggesting that the differential equation controlling generation–recombination under light is
dn
= F − Rr n 3
dt
Adv. Funct. Mater. 2020, 30, 1908427
(5)
Here, F is the generation rate due to incoming light, and Rr
is a constant controlling the recombination rate. This dependence is further confirmed by the photocurrent vs light power
dependence (Figure 3a). Assuming that steady state is reached
for these measurements (dn/dt = 0), by solving Equation (5) we
find a dependence as Iph ∝ n ∝ Fϑ, with ϑ = 1/3. In fact, the fits
shown in Figure 3a yield ϑ625 = 0.324 ± 0.003, ϑ530 = 0.318 ±
0.004, ϑ455 = 0.293 ± 0.013, confirming this prediction.
The observed power-law dependence is related to the
dynamics of the traps and recombination centers that enable
the photoconduction in nanostructured materials. A nonlinear
dependence of the photocurrent on the light intensity can arise
from the distribution of traps and recombination centers within
the band gap[95,96] and the saturation of these states under
strong light excitation,[13,18,97–99] or even from the presence of
a space charge region.[100,101] The particular case of the thirdorder equation, as suggested in ref. [30], can be related to the
recombination assisted by doubly charged Se vacancies, which
have been observed in our sample by EDX analysis and by previous studies on β-InSe.[69,84,85]
We remark that doubly charged vacancies in CdS have been
related to more complex processes involving not only charge
excitation, but also charge-lattice coupling that lead to a thermally activated recombination behavior,[30] suggesting that further studies of these properties can lead to interesting physics
of the material.
3. Conclusion
We demonstrated that spray-coated liquid phase exfoliated
β-InSe photodetectors have good photosensitive responsivity
to visible and NIR (<900 nm) light and can be used as semiconductor channel material in phototransistors, obtaining
a high-throughput and low-cost method to implement βInSe photodetectors with high sensitivity (maximum D*
≈5.49 1012 Jones, Rph ≈ 274 A W−1 at 455 nm illumination) and
fast response time (τR ≈ 15 ms, τF 64 ms). These FoM represent
an improvement of over one order of magnitude with respect
to reported photodetectors based on percolating networks of
solution processed 2D flakes[18] and are competitive with the
values reported for transition metal dichalcogenide single
flake devices.[91] The use of spray coating and environmentally
friendly solvents in the fabrication process makes this material
an interesting alternative for photodetectors in the visible and
NIR spectral range, also for applications on flexible substrates.
The gate tuneable transport and the cubic photo-charge recombination law behavior observed in β-InSe nanoflakes films
prompt further fundamental studies of this mesoscopic system.
4. Experimental Section
Exfoliation of Bulk β-InSe: β-InSe single crystals were grown by the
modified Bridgman–Stockbarger method, as described elsewhere.[73] A
quantity of 40 mg of β-InSe was exfoliated in 20 mL IPA (ACS Reagent,
≥99.8%, Sigma-Aldrich) through LPE[42] in a sonic bath (6 h, 25–35 °C,
Branson 5800 cleaner, Branson Ultrasonics), followed by SBS[102]
(1000 × g for 30 min at 15 °C, Beckman Coulter Optima XE-90) and
collection of the supernatant (≈80%), as described in ref. [69].
1908427 (7 of 10)
© 2020 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
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www.afm-journal.de
Material Characterization: The extinction spectra of the exfoliated InSe
flake dispersions in IPA diluted 1:10 was measured using a Cary Varian
5000 UV–vis, subtracting the extinction of pure solvent.
TEM analysis was carried out on a JEOL JEM 1400Plus microscope
(120 kV), with a LaB6 source, a Gatan CCD camera Orius 830. Samples
were prepared by drop-casting the flake dispersions onto carbon-coated
Cu grids and dried overnight in vacuum.
The XPS analysis was performed on a Kratos Axis UltraDLD
spectrometer at a vacuum better than 10−8 mbar, using a monochromatic
Al Kα source operating at 20 mA and 15 kV and collecting photoelectrons
from a 300 × 700 µm2 sample area. Wide spectra were acquired at pass
energy of 160 eV and energy step of 1 eV, while high-resolution spectra
were acquired at pass energy of 10 eV and energy step of 0.1 eV. The
samples were prepared by drop-casting the dispersion of InSe flakes
onto Au-coated Si chip in N2 atmosphere, while heating the substrate
to 60 °C. Bulk InSe crystals were sticked onto conductive carbon tape
and cleaved prior analysis. The samples were transferred to the XPS
chamber in inert atmosphere. Data analysis was carried out with
CasaXPS software (version 2.3.19PR1.0). The energy scale was calibrated
by setting the C 1s peak at 284.8 eV.
UPS was performed with He I (hν = 21.2 eV) radiation to obtain the
workfunction and the position of the valence band maximum of the
materials under investigation. The experiments were carried out on the
samples after the XPS analysis using the same equipment. A −9.0 V bias
was applied to the sample in order to determine the low kinetic energy
cut-off.
AFM images of the samples were acquired using a Nanowizard
III (JPK Instruments, Germany) mounted on an Axio Observer D1
(Carl Zeiss, Germany) inverted optical microscope, using PPP-NCHR
cantilevers (Nanosensors, USA). Samples were prepared by dropcasting the exfoliated InSe flake dispersions onto mica sheets (G250-1,
Agar Scientific Ltd., Essex, UK). The images (512 × 512 data points) of
5 × 5 µm2, 2.5 × 2.5 µm2, and 500 × 500 nm2 were collected at a scan rate
of 0.6 Hz in intermittent contact mode by keeping the set point above
65% of the free oscillation amplitude. Height profiles of ≈100 flakes were
analyzed with JPK Data Processing software (JPK Instruments, Germany).
Raman spectroscopy measurements were carried out with excitation
wavelength of 514.5 nm and incident power of 1 mW, using a Renishaw
micro-Raman InVia system equipped with a 100× objective. The samples
were prepared by drop-casting InSe flake dispersions on Si/SiO2
substrates and analyzed after drying in vacuum by collecting 20 spectra
in different positions. The spectra were fitted with Lorentzian functions.
For micro-photoluminescence spectra, a Renishaw inVia was used,
equipped with a 50× (0.75 N.A.) objective and laser excitation wavelength
of 785 nm. The PL spectra were recorded on films deposited on quartz
with a time exposure of 10 s and laser power ≈1 mW. The bulk sample
was measured with a time exposure of 1 s and laser power of ≈50 µW.
The crystal structure was characterized by XRD using a PANalytical
Empyrean diffractometer with Cu Kα radiation. The samples were
obtained by deposition of InSe dispersions on Si substrates.
The viscosity of the InSe ink in IPA was measured with a Discovery
HR-2 Hybrid Rheometer (TA instruments), using a double-wall concentric
cylinders geometry (inner diameter of 32 mm and outer diameter of
35 mm), designed for low-viscosity fluids. The temperatures of the inks
were set and maintained at 25 °C throughout all the measurements.
The SEM/EDX measurements on the devices were performed using
a Helios Nanolab 600 (FEI Company) combined with an X-Max detector
and INCA s system (Oxford Instruments) for the EDX spectra acquisition
and analysis. For SEM measurements an accelerating voltage of 10 kV
and beam current of 0.2 nA were used, while for EDX measurement
these values were set to 10 kV and 0.8 nA. The sample was imaged as it
was, without any conductive coating applied to the surface.
Device Fabrication: A set of nine interdigitated source/drain
electrodes for FETs were patterned on a highly p-doped Si chip covered
with a 100 nm layer of thermal oxide. Each source/drain electrode
pair consisted of 65 pairs of interdigitated fingers with an overlap of
40 µm and a gap L = 1 µm, which resulted in an overall channel width
W = 5160 µm and an active area of W × L = 5160 µm2 for photodetection.
Adv. Funct. Mater. 2020, 30, 1908427
Source (S) and drain (D) contacts were patterned by EBL with
poly(methyl methacrylate) (PMMA) resist, metal e-beam evaporation
(5 nm Ti/30 nm Au) using magnets to not expose the PMMA, followed
by lift-off. The device was completed by spraying the entire surface of the
chip with ≈30 mL of the β-InSe ink in IPA, while heating the substrate
to 60 °C in air. The coated sample was placed under vacuum overnight
at room temperature and then annealed at 200 °C for 30 min in argon.
Device Characterization: Electrical characterization was performed at
room temperature in vacuum, using a shielded probe station equipped
with a Keithley 2612 source meter with two channels to control both
the drain and the gate bias potential with respect to the source terminal
of the device. To keep its stability and reduce the effect from surface
adsorbates, the device was measured under vacuum (≈10−5 mbar). The
backside of the doped silicon substrate was electrically contacted to a
gold pad with silver paint to work as the gate electrode. The measurement
procedure was controlled by a PC using a program witten in LabVIEW
(National Instruments). For the photoresponse measurements, LEDs with
nominal wavelength of 455, 530, and 625 nm (M455L3, M530L3, M625L3
Thorlabs) were used. Light was focused on the device with a collimating
lens. The LED output power was controlled by the power supply (LEDD1B
Thorlabs). Before measuring the device, the irradiance at the center of the
focused light spot was determined with the following procedure: the light
was focused on a pinhole (⌀ = 3.37 mm) and the power of the transmitted
light was measured with a silicon photodiode (S120VC, Thorlabs)
connected to a power meter (PM100D, Thorlabs), allowing the calculation
of the irradiance at the center of the spot by dividing the power by the area
of the pinhole. A 10% loss due to the reflection of the optical window of
the vacuum probe station was taken into account for the calculation.
Spectral measurements were performed with a Xe lamp coupled to
a Spectral Products CM110 monochromator. The light was modulated
by a mechanical chopper at 23 Hz and the AC current was measured
with a Signal Recovery DSP 7265 lock-in after amplification by a DL1211
current amplifier. The same setup was used for frequency modulation
measurements.
Supporting Information
Supporting Information is available from the Wiley Online Library or
from the author.
Acknowledgements
N.C. and M.S. contributed equally to this work. N.C. gratefully
acknowledges the financial support of a Ph.D. scholarship from Region
Sardinia (P.O.R. Sardegna, European Social Fund 2007–2013—Axis IV
Human Resources, Line of Activity I.3.1). The authors thank the Clean
Room Facility of the Italian Institute of Technology for support with
device fabrication and Dr F. De Angelis (Plasmon Nanotechnologies
group) for the access to the Raman equipment.
Conflict of Interest
The authors declare no conflict of interest.
Keywords
2D semiconductors, field effect transistors, indium selenide, liquid phase
exfoliation, photodetectors, solution processed, spray coating
1908427 (8 of 10)
Received: October 12, 2019
Revised: January 5, 2020
Published online: February 14, 2020
© 2020 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
www.advancedsciencenews.com
www.afm-journal.de
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