Open Access Article
Prabhukrupa Chinmay
Kumar
a,
Subhashree
Mohanty
b,
Swikruti
Supriya
a,
Rojalin
Swain
c,
Jagadish
Kumar
cd and
Ramakanta
Naik
*a
aDepartment of Engineering and Materials Physics, Institute of Chemical Technology, Indian Oil Odisha Campus, Bhubaneswar, 751013, India. E-mail: ramakanta.naik@gmail.com
bFaculty of Science, Sri Sri University, Cuttack, 754006, India
cDepartment of Physics, Center of Excellence in High Energy and Condensed Matter Physics, Utkal University, Bhubaneswar 751004, India
dDepartment of Physics and Astrophysics, University of Delhi, Delhi-110007, India
First published on 13th January 2026
Photodetectors play a pivotal role in recently developed optical communication and imaging systems. Metal chalcogenide-based photodetectors are widely used for visible light photodetection. In this regard, a combined heterostructure of In2Se3 and Ag2S is a promising candidate for visible light photodetection. The annealing-induced Ag2S diffusion into the In2Se3 layer resulted in a high-performance photo detectivity performance of 7.32 × 109 Jones. It showed the highest photocurrent of 62.35 nA during the rise phase and 67.74 nA during the decay phase, coupled with strong Ion/Ioff ratios of 3.96 (rise) and 3.18 (decay). Its rise and fall times (τr = 7.15 and τd = 6.35 s) were moderate and well-balanced, suggesting efficient charge separation and recombination kinetics. The bandgap of the annealed film increased with reduction in structural disorder, as evidenced by UV-visible spectroscopy and well supported by DFT results. The amorphous to polycrystalline phase transformation induced a change in surface morphology and reduced the contact angle, thereby decreasing hydrophobicity. The refractive index decreased with an increase in optical transmission and skin depth, while optical density reduced upon annealing. X-ray photoelectron spectroscopy revealed the oxidation states of the elements, while energy-dispersive X-ray analysis presented the elemental composition of the films. The heterostructure formation and its mixing upon annealing were evident from the cross-sectional FESEM images, and the presence of the planes was confirmed through HRTEM images. The observed optical properties, along with enhanced photodetection, pave the way toward the construction of novel III–VI metal chalcogenide-based heterojunctions for high-performance and broadband photodetectors.
Compounds formed from the binary combinations of IIIA–VIA group elements, basically In-based alloys, such as In2S3, InSe, and In2Se3, have great importance and are widely used in photodetection applications.9–11 The important aspects of these combinations include controlled morphology, tunable bandgap, flexibility, good stability, 2D structure, carrier mobility, and remarkable fundamental properties. The 2D materials also have very good light–matter interactions and excellent optoelectronic properties. However, in recent times, heterostructure films have been widely used for photodetector applications over a broad wavelength range. For a wider spectral range, stacking α-In2Se3 with any 2D semiconducting alloy is a good choice for achieving speedy photo response. The α-In2Se3/Si heterojunction acts as a highly efficient heterojunction-based photodetector for photoelectric imaging and object recognition.12 The α-In2Se3/Ta2NiSe5 heterojunction-based photodetector works in both bias voltage state and self-driven state. The detection waveband covers between 405–1550 nm with a response time of only 25 µs.13 The α-In2Se3/WSe2 heterostructure-based photodetector has detectivity and photoresponsivity of 4.34 × 1014 Jones and 4.61 × 105 A W−1, respectively.14 The self-powered γ-In2Se3/p-Si heterojunction-based photodetector has enhanced photoresponsivity of 47.9 mA W−1, photosensitivity of 282, and photo detectivity of 8.45 × 1010 Jones. The heterostructure explores humidity and light-intensity-dependent photo response.15 The partially gated MoS2/α-In2Se3 heterojunction photodetector shows excellent photo response performance and a non-volatile photo memory effect. This is suitable for applications like non-volatile memory and other optoelectronic applications involving the design of 2D ferroelectric devices.16 The photo response in the 650–900 nm range is shown by a WSe2/In2Se3 heterojunction-based photodetector with good optoelectronic performance at room temperature. The direct band gap multilayer material-based 2D vdW heterojunctions are suitable for future optoelectronic devices.17 The photo response of the In2Se3/MoS2 heterojunction photodetector is up to 1310 nm. Here, the photocurrent generation mechanism shifts from photogating to photoconductive effect.18 The observation of no persistent photoconductivity with a fast transient response is observed in the p-GaN/α-In2Se3 heterojunction-based UV/Near-IR dual-band photodetector. The formation of α-In2Se3, along with a wide bandgap semiconductor-based heterostructure, is used for a special type of optoelectronic device.19
Different energy treatments that can lead to better performance in such a heterostructure include ion irradiation, laser irradiation, and annealing.20–22 In2Se3/p-Si heterojunction photodetectors show enhanced performance with increasing argon ion fluence. It brings out higher photosensitivity, photoresponsivity, and photo detectivity with faster rise and decay times. It shows good response to radiation hardening and is used for developing space-based photodetectors.20 The excitation wavelength of 638 nm at 10 nW laser power and 1500 s with an In2Se3/PtSe2 photodetector resulted in a fast response broadband photodetector. Such a photodetector is suitable for low-energy consumption and high-capacity optoelectronic devices.21 The thermal annealing on an SnS-based thin film resulted in a specific detectivity of 6.8 × 1010 Jones, which is nearly two orders of magnitude greater than that of the unannealed film.22 In our earlier work, the annealing effect on an 800 nm Ag2S-based In2Se3 heterostructure film resulted in remarkable photodetection ability with 2.01 × 10−1 A W−1 responsivity and detectivity of 7.32 × 109 Jones. The nA to mA current increase with annealing at 250 °C dramatically enhanced the photo response.23 The current study relies on a low-thickness Ag2S/In2Se3 heterojunction thin film annealed at various temperatures to probe the optimized performance. The annealed heterostructure was subjected to various experimental tools like X-ray diffraction (XRD), X-ray photoelectron spectroscopy (XPS), cross-sectional field emission scanning electron microscopy (FESEM), and photo response studies. The experimental results are supported by density functional theory (DFT) based calculations.
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| Fig. 1 Cross-sectional FESEM images of the (a) as-deposited and (b) annealed films. (c) XRD patterns. | ||
XRD analysis, as depicted in Fig. 1(c), reveals a significant transformation in the structural properties of the Ag2S/In2Se3 thin films upon thermal annealing. The as-prepared films demonstrate an amorphous structure, lacking the long-range atomic order characteristic of crystalline materials. In contrast, the application of heat treatment promotes the development of a polycrystalline structure, indicating the formation of distinct crystalline grains within the material. This enhancement in crystallinity is directly proportional to the annealing temperature, suggesting that higher thermal energy facilitates more ordered atomic arrangements and grain growth.23 The increased annealing temperature also encourages interdiffusion between the Ag2S and In2Se3 phases, potentially leading to the formation of new or mixed phases. The XRD patterns of the annealed thin films exhibit several characteristic diffraction peaks, signifying the presence of multiple crystalline phases. Specifically, peaks observed at approximately 26.21°, 43.88°, and 51.92° are attributed to the cubic AgInSe2 phase, correlating with the (1 1 1), (2 2 0), and (3 1 1) crystallographic planes, respectively (ICDD: 00-023-0636). Additionally, a peak detected around 25.43° corresponds to the (1 1 2) plane of the tetragonal AgInS2 phase (ICDD: 01-075-0117). The crystallite size, denoted as D, represents the extent of coherent diffraction within the thin films for each specific diffraction peak, essentially reflecting the grain size in a polycrystalline material. This critical structural parameter can be quantitatively determined using Scherrer's equation, which correlates the crystallite size to the broadening of XRD peaks.
The crystallite size, often symbolized as D, refers to the dimensions of the coherently diffracting domains within a thin film and is expressed as,
![]() | (1a) |
Lattice strain (ε) quantifies the deformation in the dimensions of a crystal lattice relative to its unstrained state. This strain can manifest in two primary forms: uniform and non-uniform strains. Uniform strain involves a consistent expansion or contraction of the unit cell across the entire crystalline volume. While uniform strain does not contribute to the broadening of diffraction peaks, it causes a shift in peak positions and an alteration in the calculated lattice parameters.25 This shift is a direct indicator of the average change in interplanar spacing. The lattice strain is calculated using the following equation,26
![]() | (1b) |
Dislocation density (δ) is a fundamental microstructural parameter defined as the total length of dislocation lines per unit volume of a crystalline material. While dislocations are non-equilibrium defects, meaning they are not inherently stable according to thermodynamic principles, their observable density holds significant importance in influencing a material's macroscopic properties.27 These linear crystallographic defects play a crucial role in plastic deformation, strengthening mechanisms, and various other physical phenomena in solids.28
![]() | (1c) |
The quantity of crystallites within a material, often denoted as the number of crystallites (NC), is primarily governed by intrinsic structural characteristics, specifically the crystallite size (D) and the extent of agglomeration or clustering among these crystalline domains. These structural factors directly influence how many individual crystallites are present in a given volume or area of the material. A smaller average crystallite size generally implies a larger number of crystallites for a constant material volume and can be calculated as,
![]() | (1d) |
The calculated structural parameters are summarized in Table 1. The crystallite size (D) increases progressively with annealing temperature. This enhancement can be attributed to the additional thermal energy that promotes recrystallization and re-nucleation, thereby improving the degree of crystallinity. Densification promotes the development of small nuclei during annealing, which eventually expand and unite to form bigger, more structured crystallites. As a result, numerous crystallites are generated, leading to an increased effective surface area for light absorption. This structural modification favors stronger light–matter interaction, thereby reducing the optical bandgap through enhanced absorption relative to transmission.29,30
| Structural parameters | Asp | 150 °C | 150 °C | 200 °C | 250 °C |
|---|---|---|---|---|---|
| D (nm) | Amorphous | Amorphous | 15.820 | 17.320 | 18.156 |
| δ (×1015 m−2) | — | — | 0.004 | 0.003 | 0.006 |
| Lattice strain (ε) | — | — | 0.010 | 0.009 | 0.007 |
| N C (nm−2) | — | — | 0.151 | 0.115 | 0.100 |
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| Fig. 2 TEM images at (a) 100 nm and (b) 50 nm. (c) HRTEM view and (d) SAED pattern of the 250 °C-annealed Ag2Se/In2Se3 thin film. | ||
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| Fig. 3 FESEM images of the (a) as-prepared and (b)100 °C-, (c) 150 °C-, (d) 200 °C-, and (e) 250 °C-annealed films. | ||
The presence of elements after film preparation and annealing is confirmed through EDS data. The film annealed at 250 °C shows different elemental peaks, indicating the presence of related elements. The unassigned peaks refer to the carbon and gold peaks. Carbon tape and gold coating were used to avoid charging of the film, as the films were coated on a glass substrate. Fig. 4(a) shows the peaks for Ag, In, S, and Se, thus confirming the presence of these elements in the film after annealing. The EDS pictures of the pristine and other annealed samples are depicted in Fig. S2. The elemental distribution indicates the uniformity of the film as illustrated in Fig. 4(b–e). The atomic% values obtained from the EDS peaks of Ag, In, S and Se for each thin film sample are shown in Table S1.
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| Fig. 4 (a) EDS spectra and elemental mapping of (b) Ag, (c) Se, (d) In, and (e) S in a 250 °C annealed film. | ||
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| Fig. 5 XPS analysis: (a) survey spectra and (b) Ag 3d, (c) Se 3d, (d) S 2p, and (e) In 3d spectra of the 250 °C-annealed Ag2S/In2Se3 thin film. | ||
Further detailed analysis of the core-level spectra reveals specific chemical environments for each element. As depicted in Fig. 5(b), the Ag 3d core level spectrum exhibits a doublet, characteristic of spin–orbit splitting, with peaks observed at approximately 367.46 eV (Ag 3d5/2) and 373.50 eV (Ag 3d3/2) with a binding energy of 5.97 eV.31 These binding energies are indicative of metallic silver (Ag (0)). Furthermore, the Se 3d peak, presented in Fig. 5(c) at around 53.95 eV, signifies spin–orbit coupling characteristics typical for selenium in this particular thin film. Similarly, the S 2p peak, shown in Fig. 5(d), presents a doublet structure at around 160.12 eV (S 2p3/2) and 165.83 eV (S 2p1/2), confirming the presence of sulfur in a specific chemical state within the film with a binding energy of 5.81 eV. Finally, the In 3d spectrum, illustrated in Fig. 5(e), displays two distinct peaks at approximately 444.61 eV and 452.21 eV, corresponding to the In 3d5/2 and In 3d3/2 components, respectively. These values are consistent with indium in a compound form. These detailed core-level analyses collectively provide critical insights into the chemical states and bonding environments of the constituent elements in the Ag2S/In2Se3 thin films.32–34
![]() | (2a) |
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| Fig. 6 Contact angle images of the (a) as-prepared, (b) 100 °C-, (c) 150 °C-, (d) 200 °C-, (e) 250 °C-annealed films. | ||
The evaluated values in Table 2 indicate an increase in surface free energy with heat treatment. The value of γse was 7.791 mN m−1 for the bilayer film, which increased to 12.289 mN m−1 after annealing at 250 °C. The work of adhesion (Wsl) was calculated from the Young–Dupré equation.37
Wsl = γw(1 + cos θ) | (2b) |
| Parameters/irradiation (min) | As-prepared | 100 °C | 150 °C | 200 °C | 250 °C |
|---|---|---|---|---|---|
| θ C (degree) | 110° | 108° | 105° | 102° | 100° |
| γ se (mN m−1) | 7.791 | 8.593 | 9.886 | 11.291 | 12.289 |
| W sl (mN m−1) | 47.367 | 49.743 | 53.357 | 57.022 | 59.489 |
.42 Here, T stands for transmittance, and ‘t’ is the film thickness. Fig. 7(b) shows the reduction in absorption upon annealing. This physical quantity is essential for evaluating other necessary constants. The stability of the absorption coefficient at higher wavelengths signifies the normal dispersion behaviour.
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| Fig. 7 Variation in (a) transmission, (b) absorption coefficient, (c) bandgap, (d) optical density, (e) skin depth and (f) extinction coefficient with annealing conditions. | ||
The bandgap (Eg) depends on the value of ‘α’ along with the incident photon energy through the Tauc relation.43
| (αhv) = C(hv − Eg)w | (3) |
The kind of transition between the valence and conduction bands depends on the exponent ‘w’ value. The direct and indirect allowed transition follows w = 1/2 and 2. The direct and allowed forbidden transition follows w = 3/2 and 3. The present data follow an indirect allowed transition, as illustrated in Fig. 7(c). Linear fitting of the data evaluates the Eg value from its X-intercept, and the slope determines the Tauc parameter. The individual plot is illustrated in Fig. S3. The increased Eg value for the annealed film in comparison to the bilayer film shows the intermixing effects of the two layers influencing the optical bandgap.44 The bilayer film with an Eg value of 0.816 eV showed an increased band gap to 1.311 eV after annealing at 250 °C. Such a change was explained by Davis and Mott in the so-called “density of state model”.45 The enhanced Eg value is because of the improved structural change by annealing. This is reflected in the XRD data. Such changes are due to decreased disorder as measured through the Urbach energy (EU) and Tauc constant (B1/2). The EU value is determined from the Urbach relation46
. The absorption coefficient at Eg is represented by α0. The linear fit of the absorbance data in the low-absorption regime with photon energy evaluates the EU value. From the calculation, the EU value for the bilayer structure was 543 meV, which was reduced to 432 meV for the 250 °C-annealed film. The other values are given in Table 3. Such reduced strength is the signature of increased structural order or decreased disorder.46 The other parameter B1/2 is inversely related to EU, as shown by the increased value reported in Table 3.47 The annealing-induced saturated bond formation resulted in the reduction of defect states.48 This implies an improvement in structure in terms of microstructural order inside the film.
| Optical parameter | As-prepared | 100 °C | 150 °C | 200 °C | 250 °C |
|---|---|---|---|---|---|
| Optical band gap (eV) | 0.816 | 0.903 | 1.017 | 1.162 | 1.311 |
| Tauc parameter (cm−1/2 eV1/2) | 243 | 267 | 298 | 321 | 344 |
| Urbach energy EU (meV) | 543 | 512 | 489 | 465 | 432 |
| σ (×10−2) | 4.761 | 5.048 | 5.286 | 5.559 | 5.983 |
| S e–p | 14.001 | 13.205 | 12.610 | 11.991 | 11.141 |
| (ηopt) | 1.633 | 1.645 | 1.661 | 1.676 | 1.691 |
| (ε∞) | 12.852 | 12.117 | 11.303 | 10.445 | 9.715 |
| (n0) | 3.585 | 3.481 | 3.362 | 3.232 | 3.117 |
The other parameters, the steepness parameter (σ) as well as electron–phonon interaction strength (Se–p) are associated with EU.49
![]() | (4) |
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| Fig. 8 (a) Variation in Se–p and ‘σ’ with annealing temperature. (b) Refractive index at different bandgap values through various models. | ||
Optical density (OD) indicates the absorption strength of the films. It is determined from the relation, OD = α × t. The variation in OD with ‘hν’ at various annealed conditions is illustrated in Fig. 7(d). Its value decreases for the annealed film at higher temperatures. The skin depth or penetration depth (δ) is another important parameter for optical quality determination. It is equal to 1/e times the photon density at the surface state. It is associated with the conductivity of semiconducting materials. The value is determined by the reciprocal of ‘α’ (δ = 1/α).49 The increased skin depth with photon energy, as well as annealing temperature, results from the low absorbance, which enhances transmittance (Fig. 7(e)).42 The extinction coefficient
measures the loss of light during crossing through the sample by scattering and absorption. The change in k at various annealing states is presented in Fig. 7(f). It presents a lower value for the annealed film over the as-prepared bilayer film. The ‘k’ values increased with photon energy and decreased with annealing temperature.
These optical property trends with annealing confirm that improvements in transparency, bandgap, and optical constants arise from enhanced crystallinity, reduced defect states, and the formation of well-ordered AgInS2/AgInSe2 phases, all of which play a crucial role in optimizing light absorption and charge transport behavior in the thin film photodetector.
The high-frequency dielectric parameter is evaluated by εL = n2. In the present study, εL increased with irradiation time (Table 3). It is attributed to the electrical polarizability of the material and is connected with free charge carriers affecting polarization.50 The optical conductivity (ηopt) is determined by
and the values are given in Table 3.50 It measures the affinity of an atom for bond formation.51 In the present case, it increased from 1.633 (un-annealed) to 1.691 for the 250 °C-annealed film (Table 3).51
The refractive index (n) evaluates the dispersion of light waves and other nonlinear optical phenomena. The calculation of ‘n’ from Eg by using the Dimitrov and Sakka empirical relation establishes a useful connection between the electronic band state and the optical dispersion of the films52
![]() | (5a) |
![]() | (5b) |
![]() | (5c) |
![]() | (5d) |
The exponential relation of ‘n’ for semiconductors with band gaps is given by Tripathy,57 and the relation is
| nT = 1.73 × [1 + 1.9017 × e−0.539×Eg] | (5e) |
The values obtained from different models are expressed in Fig. 8(b). It presents the inverse relation with Eg.
| Sample | I L (A) | I D (A) | I L − ID (A) | Photo sensitivity (%) | Responsivity (R) (A W−1) | Detectivity (D*) (Jones) |
|---|---|---|---|---|---|---|
| Asp | 1.79 × 10−8 | 4.66 × 10−9 | 1.32 × 10−8 | 73.96 | 3.58 × 10−6 | 3.09 × 108 |
| 100 °C | 1.17 × 10−7 | 7.5 × 10−9 | 1.09 × 10−7 | 93.61 | 2.34 × 10−5 | 2.89 × 107 |
| 150 °C | 1.55 × 10−7 | 1.85 × 10−8 | 1.36 × 10−7 | 88.06 | 3.10 × 10−5 | 1.95 × 108 |
| 200 °C | 3.53 × 10−6 | 6.42 × 10−7 | 2.89 × 10−6 | 81.84 | 7.07 × 10−4 | 7.32 × 109 |
| 250 °C | 2.51 × 10−4 | 1.75 × 10−4 | 7.66 × 10−5 | 30.43 | 5.03 × 10−2 | 1.44 × 107 |
Photodetector performance under various light intensities is basically driven by the formation of electron–hole pairs proportional to the power of the incident light. Incorporating an Ag2S layer on In2Se3 increases carrier concentration in In2Se3, enhancing the overall response. Additionally, surface interactions involving oxygen play a critical role: in the dark, oxygen molecules adsorb onto the surface, capturing electrons (O2 + e−→ O2−), while under illumination, photogenerated holes trigger the desorption of oxygen, freeing electrons to the conduction band and elevating photocurrent.23 Key performance indicators such as photoresponsivity (R) and detectivity (D) were calculated by standard formulas and are also detailed in Table 41,60–62
![]() | (6a) |
![]() | (6b) |
![]() | (6c) |
The I–V characteristics of Ag2S/In2Se3 thin films, under both dark and illuminated states, demonstrate clear symmetry and a consistent increase in current under illumination across all samples. The logarithmic plots (Fig. 9(a–e)) show enhanced photocurrent (IL) compared to dark current (ID), with the 250 °C annealed sample exhibiting the highest absolute current levels. However, Fig. S4 (with a linear y-axis) reveals that while the 250 °C sample produces the highest IL and ID values, the contrast between light and dark currents, indicative of sensitivity, is reduced compared to other annealed conditions. Quantitative analysis from Table 4 supports this observation. The highest photosensitivity (93.61%) is recorded for the 100 °C sample, followed closely by the 150 °C and 200 °C samples. The 250 °C sample, despite showing the largest IL (2.51 × 10−4 A), demonstrates the lowest relative photosensitivity (30.43%) due to a high baseline dark current. Nevertheless, its responsivity (5.03 × 10−2 A W−1) and detectivity (1.44 × 107 Jones) remain significant, highlighting its utility in applications requiring high absolute photocurrent rather than contrast.
Overall, moderate annealing temperatures (100–250 °C) improve photodetection performance by optimizing light-induced carrier generation and suppressing dark current. The 200 °C sample strikes a balance, offering enhanced current response, high responsivity (7.07 × 10−4 A W−1), and the best detectivity (7.32 × 109 Jones), attributed to improved crystallinity and reduced surface recombination.
A comparative analysis of films annealed at different temperatures reveals that photoresponsivity (R) correlates strongly with the films' structural and optical properties. As the annealing temperature increases from 100 °C to 200 °C, enhanced crystallinity, improved interfacial uniformity, and reduced defect density collectively enhance carrier mobility and light absorption, leading to higher R and D values. However, further annealing to 250 °C introduces excess charge carriers and defect-assisted conduction pathways, increasing dark current and reducing photosensitivity. Thus, the 200 °C annealed film achieves the optimal balance between crystallinity, defect control, and interfacial quality, resulting in the highest responsivity and detectivity among all samples.
However, the rise in dark current at 250 °C indicates that excessive annealing increases carrier concentration and defect-assisted conduction, thereby reducing photosensitivity. This demonstrates that optimal photodetector performance arises not from maximum current output but from a balanced combination of crystallinity, defect density, and interfacial integrity conditions best achieved at 200 °C. Table S2 compares the key photodetection parameters of the present Ag2S/In2Se3 device with those of other 2D/In2Se3-based systems reported in the literature. The results demonstrate that the optimized Ag2S/In2Se3 heterostructure exhibits comparable responsivity and detectivity, while offering a broader visible spectral response due to efficient interfacial charge transfer and reduced recombination losses.
Fig. 10(a–c) displays the I–T curves for Ag2S/In2Se3 films annealed at 150 °C, 200 °C, and 250 °C under bias voltages of 5, 7.5, and 10 V, showing distinct on/off light cycles. All samples exhibit a sharp increase in current upon illumination, followed by a quick drop when the light is off, driven by enhanced carrier drift velocity. The increased photocurrent at higher bias voltages is attributed to stronger electric fields, which improve charge separation, reduce recombination, and expand the depletion region, leading to more efficient carrier generation and collection. Variations in maximum current among samples are likely influenced by defect states. After the light is off, the photocurrent decreases due to recombination between trapped and free carriers, with additional effects from non-radiative processes and carrier transport variations. For consistent analysis, a specific peak within the 60–150 second interval is selected for all samples, as shown in Fig. 10(d–f). From this peak, key parameters, such as light-on (Ion), light-off (Ioff), and Ion/Ioff ratios during rise and decay phases, are extracted and presented in Table 2 to evaluate photodetector performance.
Furthermore, the transient photoresponse (I–T) curves in Fig. 10(a–c) show that the photocurrent quickly returns to its baseline after each illumination cycle, indicating the absence of persistent photoconductivity. This behavior reflects efficient carrier recombination and minimal trap-assisted retention, confirming the fast and reversible photoresponse characteristics of the Ag2S/In2Se3 heterostructure.
Rise time (τr) and decay time (τd) are essential indicators of a photodetector's responsiveness. The rise time measures how quickly the current increases (from 10% to 90%) when light is applied, while the decay time reflects how fast it returns to baseline (from 90% to 10%) after light is removed. Shorter τr and τd values indicate faster response and recovery, which are critical for high-speed light detection.5 These parameters, extracted from Fig. 10(d–f), are presented in Table 5 to evaluate the dynamic performance of Ag2S/In2Se3 photodetectors.
| Sample | During rise | During decay | ||||||
|---|---|---|---|---|---|---|---|---|
| I on (nA) | I off (nA) | I on/Ioff | τ r (s) | I on (nA) | I off (nA) | I on/Ioff | τ d (s) | |
| 150 °C | 25.88 | 9.08 | 2.85 | 6.9 | 25.92 | 11.26 | 2.3 | 7.13 |
| 200 °C | 62.35 | 15.72 | 3.96 | 7.15 | 67.74 | 21.25 | 3.18 | 6.35 |
| 250 °C | 10.14 | 6.71 | 1.51 | 2.86 | 11.24 | 8 | 1.4 | 5.02 |
Fig. 10 and Table 5 present the temporal photo response behavior of Ag2S/In2Se3 films annealed at 150 °C, 200 °C, and 250 °C under different bias voltages (5, 7.5, and 10 V). All samples show a repetitive and reversible change in current upon cyclic illumination, indicating stable photodetector operation. The response amplitude increases with higher bias voltage, especially evident in the 200 °C sample (Fig. 10(b)), which exhibits the highest photocurrent. The extracted photodetector parameters (Table 5) reveal that the 200 °C sample demonstrates the most favourable characteristics overall. It showed the highest photocurrent of 62.35 nA during the rise phase and 67.74 nA during the decay phase, coupled with strong Ion/Ioff ratios of 3.96 (rise) and 3.18 (decay). Its rise and fall times (τr = 7.15 s, τd = 6.35 s) are moderate and well-balanced, suggesting efficient charge separation and recombination kinetics. The optimal dynamic behavior at 200 °C arises from a well-balanced microstructure, where enhanced crystallinity and controlled interdiffusion reduce trap-assisted recombination, thereby enabling faster carrier transport and recovery compared to under- or over-annealed films.
Fig. S5 illustrates the current–time (I–T) stability behavior of the Ag2S/In2Se3 thin films annealed at 150 °C, 200 °C, and 250 °C under continuous illumination for 1 hour (3600 s). All three samples exhibit a steady photocurrent response with minimal fluctuation, confirming good temporal stability. The photocurrent initially increases slightly before reaching saturation, which can be attributed to the gradual stabilization of charge trapping and de-trapping processes at the film–electrode interface. The 200 °C annealed sample shows the most stable and consistent current output, with negligible drift over time, indicating robust charge transport and minimal defect-mediated recombination. In contrast, the 250 °C film exhibits higher absolute current but with a slow saturation trend due to increased defect density. Overall, the I–T stability analysis confirms that the Ag2S/In2Se3 heterostructures maintain stable photocurrent characteristics over prolonged operation, particularly for the optimally annealed 200 °C sample.
In contrast, the 250 °C sample exhibits the fastest response (τr = 2.86 s) and decay (τd = 5.02 s) but suffers from reduced current contrast (Ion/Ioff ≈ 1.5), indicating lower sensitivity. Meanwhile, the 150 °C sample shows a moderate current level and contrasts with longer response times (τr = 6.9 s, τd = 7.13 s), suggesting slower carrier dynamics. Overall, the 200 °C-annealed film stands out as the optimal candidate, combining high photocurrent, strong on/off contrast, and reasonable response times, ideal attributes for practical photodetector applications. Although wavelength-dependent photoresponse measurements could not be performed due to the unavailability of a monochromatic light source, the use of a broad-spectrum white LED ensures uniform excitation across the visible region. The strong absorption and rapid transient response observed confirm the film's potential for broadband visible photodetection. Future work will include detailed spectral responsivity analysis using tunable light sources.
:
3 and a single layer of Ag–S–Se–In) have been calculated using the full potential linearized augmented plane wave (FP-LAPW) within the framework of DFT using the MedeAVASP package.63,64 DFT was used to obtain an understanding of atomistic-scale interactions that determine the various physical properties of a material. The heterostructures were constructed along the (1 0 0) plane of Ag2S and the (2 −1 0) plane of In2Se3 with a 15 Å vacuum region given along the z-direction using the VESTA visualisation software.65 The correlation and exchange energies were evaluated within the GGA by Perdew–Burke–Ernzerhof (PBE) parametrization.66 Finally, the Hubbard correction values, Ud = 4 for Ag and Up = 10 for In, Se, and S atoms, were added to enhance the localization and short-range interactions. The self-consistent calculations were performed with a self-consistent field (SCF) energy convergence threshold of 10−6 eV and a planewave cutoff of 258.689 eV. The Brillouin zone was integrated with a 2 × 2 × 1 Monkhorst–Pack grid, and the Gaussian scheme with a broadening of 0.003 Ry was used in the calculation. The band structure was calculated along the F-Γ-B-G-Γ high symmetry directions, and the corresponding density of states is depicted in Fig. 11(a–c). The conduction band is dominated by Se-4p and In-5s atoms in a 1
:
3 layer, but in the 1
:
1 case, mostly by Se-4p atoms, and the valence band is occupied by Se-4p and S-3p in a 1
:
3 layer, whereas in a 1
:
1 layer, it is occupied by Se-4p near the Fermi level. This indicates that stronger interaction or bonding is more likely in Se, In, and S atoms. The band gap (Eg) for a 1
:
3 proportion heterostructure layer of Ag2S and In2Se3 is 0.78987 eV, whereas that for a single layer of Ag–S–Se–In is 1.37339 eV. The contour plot of electron charge density shows that more charge is accumulated around the Se atom in both cases, which shows that the Se atom plays a crucial role in the materials' properties [Fig. 12].
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Fig. 11 Calculated band structures and the corresponding density of states of a (a and b) 1 : 3 proportion layer of the Ag2S/In2Se3 heterostructure and (c and d) single layer of Ag–S–Se–In. | ||
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Fig. 12 Contour plot for the charge density of a (a) 1 : 3 proportion layer of the Ag2S/In2Se3 heterostructure and (b) single layer of Ag–S–Se–In. | ||
A similar simulation was implemented for optical parameter calculations, such as the real and imaginary parts of the dielectric constant, real and imaginary parts of conductivity, reflectivity, refractive index, attenuation coefficient, extinction coefficient, and absorption, within the 0–20 eV photon energy range.
The optical parameters of a material are crucial to investigate an excellent candidate for photovoltaic and optoelectronic applications. When the matter interacts with the electromagnetic radiation, it gets polarized by the applied electric field. It affects its interaction with electromagnetic waves. Fig. 13(a and b) illustrates the real and imaginary parts of the dielectric parameter. The imaginary component, indicating the material's absorption of electromagnetic radiation, denotes the energy loss per unit volume. This aspect is directly linked to electronic transitions between unoccupied and occupied states within the sample. The real part presents peaks at ∼1.13 eV and 1.78 eV for hetero and single layers of Ag–S–Se–In, respectively. Then, it decreased with increased photon energy. Within the zero-frequency range, the static dielectric constant for the heterolayer is 3.34, whereas for a single layer, it is 1.98. Fig. 13(c) depicts the maximum absorption coefficient values at a photon energy of 9.1 eV for hetero and 4.8 eV for a single layer of Ag–S–Se–In.
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Fig. 13 Ag2S/In2Se3 heterostructure (1 : 3 and 1 : 1 proportions): (a) real part and (b) imaginary part of the dielectric function, (c) absorption coefficient, and (d) optical conductivity. | ||
Optical conductivity, extinction coefficient, attenuation coefficient, and refractive index are displayed in Fig. 14(a–d) for both the hetero layer and the single layer of Ag–S–Se–In. Fig. 14(d) indicates around 8% of reflectance for the heterolayer and 3% of reflectance for the single layer at 0 eV.
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Fig. 14 Ag2S/In2Se3 heterostructure (1 : 3 and 1 : 1 proportions): (a) extinction coefficient, (b) attenuation coefficient, (c) refractive index, and (d) reflectivity. | ||
It should be noted that the computational model represents an atomically thin Ag–S–In–Se heterostructure, designed to approximate the local interfacial environment between Ag2S and In2Se3 layers. This simplified configuration allows accurate insight into charge transfer, electronic coupling, and band alignment at the junction, which governs the experimentally observed optoelectronic behavior, even though it does not replicate the full experimental film thickness.
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