Optical and Photosensitive Properties of Flexible n (p)–InSe/In2O3 Heterojunctions

In this work, optical, including photoluminescence and photosensitivity, characteristics of micrometer-sized flexible n (p)–InSe/In2O3 heterojunctions, obtained by heat treatment of single-crystalline InSe plates doped with (0.5 at.%) Cd (Sn), in a water-vapor- and oxygen-enriched atmosphere, are investigated. The Raman spectrum of In2O3 layers on an InSe:Sn substrate, in the wavelength range of 105–700 cm−1, contains the vibration band characteristic of the cubic (bcc-In2O3) phase. As revealed by EDX spectra, the In2O3 layer, ~2 μm thick, formed on InSe:Cd contains an ~18% excess of atomic oxygen. The absorption edge of InSe:Sn (Cd)/In2O3 structures was studied by ultraviolet reflectance spectroscopy and found to be 3.57 eV and ~3.67 eV for InSe:Cd and InSe:Sn substrates, respectively. By photoluminescence analysis, the influence of doping impurities on the emission bands of In2O3:Sn (Cd) was revealed and the energies of dopant-induced and oxygen-induced levels created by diffusion into the InSe layer from the InSe/In2O3 interface were determined. The n (p)–InSe/In2O3 structures display a significantly wide spectral range of photosensitivity (1.2–4.0 eV), from ultraviolet to near infrared. The influence of Cd and Sn concentrations on the photosensitivity and recombination of nonequilibrium charge carriers in n (p)–InSe layers from the heterojunction interface was also studied. The as-obtained nanosized InSe/In2O3 structures are suitable for optoelectronic applications.


Introduction
Indium monoselenide (InSe) is a typical representative of group III-VI layered materials (In and Ga monochalcogenides). Its single crystals are comprised of elementary stratified Se-In-In-Se packages, bound by van der Waals forces, much weaker than those between four monoatomic sheets inside a package, corresponding to an ionic-covalent (predominant) bonding [1]. This allows displacement of neighboring packages relative to each other, which explains InSe polytypism and flexibility.
Being an n-type material with a room-temperature direct band gap of about 1.3 eV and an indirect one of 1.26 eV, InSe is considered, along with other classes of narrow-gap semiconductors, as a promising material for solar energy applications [2,3]. As a typical

Materials and Methods
To obtain the n-In 2 O 3 /p-InSe and n + -In 2 O 3 /n-InSe structures, single-crystalline plates of InSe doped with 0.5 at.% Cd (to get p-InSe) and 0.5 at.% Sn (n-InSe), respectively, were used. Cadmium-and Sn-doped InSe single crystals were grown by the Bridgman-Stockbarger technique. The primary InSe:Cd and InSe:Sn compounds were synthesized from component elements, In (5N) and Se (5N), which were taken in stoichiometric quantities. The respective amounts of In and Se, along with chemical elements Cd (5N) and Sn (5N), in proportions of 0.5 at.%, were introduced into quartz ampoules.
Electron and hole concentrations in n-InSe and p-InSe single crystals, at room temperature, determined from Hall effect measurements, were found to be of (4-6) × 10 16 cm −3 and 8 × 10 13 cm −3 , respectively. The preparation technology of n (p)-InSe lamellae and n (p)-InSe/In 2 O 3 structures is described in [5].
Micro-Raman spectra were recorded using a WITec RA300 microscope (excitation wavelength of 532 nm). The reflection spectra in the UV region were recorded with a Specord M-40 spectrophotometer with a spectral energy resolution of 0.5 meV, equipped with accessories for reflectance measurements at an incidence angle ≤5 • . The wavelengthmodulated reflection spectra were recorded with spectrophotometric equipment based on an MDR-2 type monochromator with 1200/600 mm −1 diffraction grating, in which one of the flat mirrors was replaced with a vibrating mirror made of Al, deposited on a 120-µm-thick Si plate with a surface area of~30 cm 2 . The vibration frequency of the mirror was 22 Hz. The wavelength resolution provided by monochromator was ∆λ = 2.5 Å.
Photoluminescence and photosensitivity spectra were registered by means of photometric equipment, including an MDR-2 monochromator, equipped with a photomultiplier with a multi-alkali [(Na2K)Sb + Cs] photocathode with a quartz window. A quartz tungsten halogen lamp with a power of 150 W was used as the excitation source of the photocurrent in the examined structures (InSe:Cd and InSe:Sn)/In 2 O 3 . The temperature of the W filament was~3300 K.
The photosensitivity of (InSe:Cd, InSe:Sn)/native oxide structures was excited with monochromatic radiation provided by a DRS-500 filtered mercury lamp (wavelength λ = 546 nm), while PL excitation was performed using a N 2 laser (λ = 334 nm) and an MRL-637 red solid-state laser with a 100 mW output power. The intensity of the laser exciting radiation was attenuated using neutral density filters with thin Pt films deposited onto amorphous quartz plates (molten SiO 2 ).
The photoresponse of p-InSe:Cd/n-In 2 O 3 heterojunctions upon bending at an angle of 15 • , in the plane perpendicular to the sample surface, was recorded on a structure formed on a plate of p-InSe doped with 0.5 at.% Cd, with a thickness of 28 µm. At the same time, a photoresistor was made based on an InSe:Cd plate with a thickness of 24 µm of the same material. Thin In films were used as electrodes. The distance between them was 6 mm, while the surface area was equal to~30 mm 2 . The thickness of the plates was calculated from the interference fringes of the transmission spectrum at wavelengths of 5-15 µm. The dependence of the photocurrent on the sample illumination using a (637 nm and 2 mW) laser radiation was studied. The beam density was~1.5 × 10 16 photons·cm −2 .

Results and Discussion
By heat treatment in air, for 6-12 h, at a temperature of 600 • C, of InSe lamellae, specially undoped and doped with Sn and Cd, their surface is covered with a purpleblue In 2 O 3 layer, displaying a poor diffuse reflection. The surface morphology of these layers was studied in [18]. The performed scanning electron microscopy (SEM) inspection revealed that the In 2 O 3 layer is composed of nanowires and nanoribbons, the length of which is tens of nanometers [5].
The X-ray diffraction (XRD) patterns of the materials obtained by heat treatment, in air, of plates with a thickness of 10-30 µm contain intense diffraction lines of the native oxide (In 2 O 3 ), together with lines of a much lower intensity of the primary material (InSe). Valuable information on the structure and chemical composition of layers formed on semiconductor and dielectric surfaces can be obtained from X-ray photoelectron spectroscopy (XPS) and energy dispersive X-ray spectroscopy (EDX) analyses [19,20]. These surface analysis techniques are based on the fact that the binding energy of atom inner shell electrons varies depending on the chemical state of the neighboring atoms. The higher the electronegativity of the neighboring atoms, the higher the ionization energy of the inner shells. Although the energy resolution of EDX spectroscopy is lower than that of XPS and auger electron spectroscopy (AES), the EDX analysis can still be used to determine the elemental composition of thin metal (Ga, Zn, In) oxide layers [18,[21][22][23][24]. Figure 1a shows the SEM micrograph for the region in close vicinity of the edge of the InSe:Cd plate (thickness 180 µm), heat-treated in air at 600 • C for 6 h. As can be clearly seen from this image, cracks and micro-defects are present on the surface oxide layer of InSe:Cd plates. The elemental composition of the layer formed on the plate surface was determined by the intensity of the characteristic lines in the EDX spectrum ( Figure 1b In [24], nanostructured In2O3 (in the form of nanowires and nanoprisms) was obtained by the calcination of In(OH)3 micro-crystallites at 350 °C for 4 h. The In/O concentration ratio was found to be 2/3, which corresponds to the stoichiometric composition In2O3. One can admit that the surplus of oxygen atoms in the In2O3 layer on the InSe substrate is determined by the high oxygen absorption capacity (from air) of the In2O3 nanowires/nanopangles formed at the temperature of 600 °C. The depth (d) of the In2O3 layer penetrated by the electron beam with energy E0 = 20 keV can be approximated using the Kanaya-Okayama empirical formula [25]: where Z is the atomic number, A denotes the mass number, and ρ is the density (g/cm 3 ). For ρ = 7.2 g/cm 3 , Z = 122, A = 278, and E0 = 20 keV, d = 2.2 μm.
Additional information concerning the chemical composition of the layer formed on the surface of the InSe:Sn plates was obtained from the analysis of Raman spectra ( Figure  2). In the wavenumber range of 60-700 cm −1 , eight vibration bands are well emphasized, of which four intense bands are located at low frequencies, 100-300 cm −1 . In refs. [26][27][28], the peak at 135 cm −1 is associated with the In-O vibrations in the InO6 octahedron, while the peak located at 306 cm −1 is attributed to the stretching vibrations of the octahedra. The 501 cm −1 and 627 cm −1 high-frequency vibration modes are interpreted in [29] as stretching vibrations in the InO6 octahedra. As can be seen from Figure 2, in the spectral range of 340-450 cm −1 , some vibration bands are missing and, instead, an intense peak at 250 cm −1 is present. In the micro-and nanostructured In2O3 layers with oxygen vacancies, a low-intensity Raman peak centered at 306 cm −1 is clearly emphasized [30]. The presence of the 250 cm −1 peak for the In2O3 layers on the InSe substrate may be caused by the excess oxygen in it. In [24], nanostructured In 2 O 3 (in the form of nanowires and nanoprisms) was obtained by the calcination of In(OH) 3 micro-crystallites at 350 • C for 4 h. The In/O concentration ratio was found to be 2/3, which corresponds to the stoichiometric composition In 2 O 3 . One can admit that the surplus of oxygen atoms in the In 2 O 3 layer on the InSe substrate is determined by the high oxygen absorption capacity (from air) of the In 2 O 3 nanowires/nanopangles formed at the temperature of 600 • C. The depth (d) of the In 2 O 3 layer penetrated by the electron beam with energy E 0 = 20 keV can be approximated using the Kanaya-Okayama empirical formula [25]: where Z is the atomic number, A denotes the mass number, and ρ is the density (g/cm 3 ). For ρ = 7.2 g/cm 3 , Z = 122, A = 278, and E 0 = 20 keV, d = 2.2 µm. Additional information concerning the chemical composition of the layer formed on the surface of the InSe:Sn plates was obtained from the analysis of Raman spectra ( Figure 2). In the wavenumber range of 60-700 cm −1 , eight vibration bands are well emphasized, of which four intense bands are located at low frequencies, 100-300 cm −1 . In refs. [26][27][28], the peak at 135 cm −1 is associated with the In-O vibrations in the InO 6 octahedron, while the peak located at 306 cm −1 is attributed to the stretching vibrations of the octahedra. The 501 cm −1 and 627 cm −1 high-frequency vibration modes are interpreted in [29] as stretching vibrations in the InO 6 octahedra. As can be seen from Figure 2, in the spectral range of 340-450 cm −1 , some vibration bands are missing and, instead, an intense peak at 250 cm −1 is present. In the micro-and nanostructured In 2 O 3 layers with oxygen vacancies, a low-intensity Raman peak centered at 306 cm −1 is clearly emphasized [30]. The presence of the 250 cm −1 peak for the In 2 O 3 layers on the InSe substrate may be caused by the excess oxygen in it.
In order to further study the chemical composition of the layer formed on the surface of the InSe:Sn plate, the Raman peak positions (in cm −1 ) from Figure 2 are summarized in Table 1. For comparison, the vibration frequencies of the rhombohedral InSe lattice [31], as well as those of the body-centered cubic In 2 O 3 in the form of nanowires [32] and nanocubes [30], were also included. As can be seen from this table, the intense bands with the maxima at 110, 135, 231, 306, and 627 cm −1 (Figure 2) are in good agreement with the Raman frequencies in the ensembles of In 2 O 3 nanoformations, identified in the works [30,32] as vibrations in cubic In 2 O 3 crystallites. The good correlation between the sets of vibration modes of the In 2 O 3 layers (Table 1, column 2) and those of the bulk In 2 O 3 single crystals (column 6) indicates that both In 2 O 3 nanowires and crystallites are present in the layer formed on the surface of the InSe:Sn plate. At the same time, the low-intensity bands positioned at 225, 475, 540, and 635 cm −1 (Table 1, column 7) are emphasized in the Raman spectrum, which have been identified in [33] as surface vibration modes in nanocrystalline SnO 2 . The 1-2 cm −1 difference between the Raman peak frequencies in the In 2 O 3 layers formed on the surface of the InSe:Sn plates and those in nanowires and nanocubes can be caused by the nature and size of the In 2 O 3 nanoformations. In order to further study the chemical composition of the laye face of the InSe:Sn plate, the Raman peak positions (in cm −1 ) from rized in Table 1. For comparison, the vibration frequencies of the rh tice [31], as well as those of the body-centered cubic In2O3 in the fo and nanocubes [30], were also included. As can be seen from this tab with the maxima at 110, 135, 231, 306, and 627 cm −1 (Figure 2) are in g the Raman frequencies in the ensembles of In2O3 nanoformations, id [30,32] as vibrations in cubic In2O3 crystallites. The good correlation vibration modes of the In2O3 layers (Table 1, column 2) and those of crystals (column 6) indicates that both In2O3 nanowires and crystalli layer formed on the surface of the InSe:Sn plate. At the same tim bands positioned at 225, 475, 540, and 635 cm −1 (Table 1, column 7) a Raman spectrum, which have been identified in [33] as surface nanocrystalline SnO2. The 1-2 cm −1 difference between the Raman pe In2O3 layers formed on the surface of the InSe:Sn plates and tho nanocubes can be caused by the nature and size of the In2O3 nanofor    Figure 3 shows the reflection spectra for an incidence angle of~5 • , in the region of the fundamental absorption edge of In 2 O 3 layers on nand p-InSe substrates. Figure 3 shows the reflection spectra for an incidence angle of ~ the fundamental absorption edge of In2O3 layers on n-and p-InSe sub The reflection factor, R, at normal incidence, for the separation su distinct optical media depends on the relative refractive and extinctio respectively, by means of the relation [34]: In the optical transparency region (λ > 380 nm), the inequality kr so that the term kr 2 can be neglected in both the numerator and the above equation [35,36]. The refractive index of the In2O3 layer depen concentration and varies between 2.17 and 1.83 for concentrations in t < 10 21 cm −3 [37]. In the considered case, putting nr ≈ 2 in Equation (2), a ≈11% is obtained for the air/In2O3 interface.
As can be seen from Figure 3 (curves 1 and 2), in the vicinity absorption edge of In2O3 crystallites, an increase by 2-3% in the ref served together with an increasing wavelength. As can be seen from and 5), in the wavelength range of 300-360 nm, the reflection spectrum on the undoped InSe substrate overlaps with that recorded for the In2 the doped substrate with 0.5 at.% Cd.
The linear region of the reflectance graphs for the In2O3 layer plates exhibits an ~15 nm redshift with respect to that formed on the plates. This displacement is clearly emphasized in the second derivativ spectra, d 2 R(λ)/Rdλ 2 .
The energy band gap in semiconductor materials can be suitabl The reflection factor, R, at normal incidence, for the separation surface between two distinct optical media depends on the relative refractive and extinction indices, n r and k r , respectively, by means of the relation [34]: In the optical transparency region (λ > 380 nm), the inequality k r 2 << (n r -1) 2 is valid so that the term k r 2 can be neglected in both the numerator and the denominator of the above equation [35,36]. The refractive index of the In 2 O 3 layer depends on the electron concentration and varies between 2.17 and 1.83 for concentrations in the range of 10 19 < N e < 10 21 cm −3 [37]. In the considered case, putting n r ≈ 2 in Equation (2), a reflection factor of ≈11% is obtained for the air/In 2 O 3 interface.
As can be seen from Figure 3 (curves 1 and 2), in the vicinity of the fundamental absorption edge of In 2 O 3 crystallites, an increase by 2-3% in the reflectance can be observed together with an increasing wavelength. As can be seen from Figure 3 (curves 3 and 5), in the wavelength range of 300-360 nm, the reflection spectrum of the In 2 O 3 layer on the undoped InSe substrate overlaps with that recorded for the In 2 O 3 layer formed on the doped substrate with 0.5 at.% Cd.
The linear region of the reflectance graphs for the In 2 O 3 layer formed on InSe:Cd plates exhibits an~15 nm redshift with respect to that formed on the surface of InSe:Sn plates. This displacement is clearly emphasized in the second derivative of the reflectance spectra, d 2 R(λ)/Rdλ 2 .
The energy band gap in semiconductor materials can be suitably determined from modulated reflection spectra (by wavelength, electric field, temperature, etc.), considering the wavelength at which the function (∆R/R) (λ) passes through zero [38]. In Refs. [36,39], the direct and indirect band gaps are determined from the spectral analysis of the function (∆R/R∆λ) (λ) in van der Waals and III-VI (GaS, GaSe, InSe) crystals. Since the photon energy for which this function passes through zero cannot be accurately determined, the property of the second derivative d 2 R(λ)/Rdλ 2 to reach its maximum (a well-pronounced peak) at a photon wavelength corresponding to the forbidden bandwidth was used. The analysis method for the particularities of the reflection spectra by means of the d 2 R(λ)/Rdλ 2 function elaborated in [35] is widely applied in the analysis of the FTIR reflection spectra.
In Figure 3 (curves 3, 4, and 6), plots of the second derivative, d 2 R(λ)/Rdλ 2 , are also presented. The maxima of respective functions are positioned at 338 nm (3.69 eV) and 347.2 nm (3.57 eV) for the reflection spectra from the In 2 O 3 layer on InSe:Sn, InSe:Cd, and undoped InSe substrates, respectively. In [40], it was established that the band gap of In 2 O 3 layers increases from 3.55 to 3.80 eV with increasing concentration of free charge carriers, from 2.6 × 10 19 to 7.0 × 10 19 cm −3 . At the same time, the electron effective mass is also increasing (>0.8 m 0 ) with the electron concentration in In 2 O 3 for n ≥ 10 19 cm −3 [41].
Indium oxide is an n-type semiconductor. Its doping with Sn contributes to the increase in the concentration of free charge carriers, while Cd as a dopant compensates the free charge carriers, thus decreasing the electron concentration in the conduction band (CB). One can consider that at low concentrations, Cd doping does not practically influence the optical band gap, E g0 (Figure 3, curve 6). The direct band gap in a heavily doped semiconductor, E gn , is given, in virtue of the Burstein-Moss model (parabolic band approximation), by [42]: where E g0 is the band gap of the undoped material; m vc * denotes the reduced effective mass of charge carriers (1/m vc * = 1/m v * + 1/m c * ) [43], with m v * and m c * representing valence band (VB) and CB effective mass, respectively;h is the reduced Planck's constant; and n is the electron concentration. Since m vc * ≥ m 0 [44], one can consider m vc * = m c * . If one admits that the optical band gap of In 2 O 3 corresponds to that of the In 2 O 3 :Cd layer (3.57 eV), then from Equation (3), with m vc * = 0.2 m 0 (m 0 -electron mass) and E gn = 3.69 eV, the electron concentration in the surface native oxide layer of InSe:Sn plates can be determined and is found to be 2.8 × 10 19 cm −3 . The electron concentration in the thin In 2 O 3 :Sn layer, determined by the Hall effect and electrical conductivity measurements, varies between 1.3 × 10 19 and 1.5 × 10 21 cm −3 [37].
The In 2 O 3 layers formed on n-InSe:Sn and p-InSe:Cd substrates are materials displaying visible photoluminescence (Figure 4a). Under laser excitation (power density 20 mW/cm 2 ) corresponding to the fundamental absorption edge of the In 2 O 3 nanocrystallite layer on a p-InSe:Cd substrate (λ = 337.4 nm (3.68 eV)), the PL spectrum (Figure 4a, curve 1) is composed of two intense bands with maxima at 440 nm (2.75 eV) and 590 nm (2.10 eV), and a low-intensity plateau located in the wavelength range of 370-400 nm, with the edge at~380 nm (3.22 eV).
Photoluminescence of micro-and nanoformations in the visible region has been the subject of many papers, especially [21,24]. The PL spectra of In 2 O 3 microcrystals cover the wavelength range of 340-500 nm, with maxima positioned at 436 nm and 447 nm, as well as a plateau at 386 nm [24]. At the same time, the PL spectrum of an ensemble of nanospheres, studied in [21], under 400 nm wavelength excitation, is composed of three bands, with peak intensities at 452, 473, and 544 nm, while at 370 nm excitation, the peak intensity of the first two bands changes, while the third band shifts to longer wavelengths by 33 nm. The structure of the PL spectrum and the energy position of the PL maxima depend on the excitation wavelength [21]. The complexity of these PL spectra in the purple-blue region is explained by different concentrations of oxygen vacancies in studied samples [21,24]. The orange-yellow PL band, with a maximum at 580-590 nm, has been observed in many papers in which different types of In 2 O 3 nanoformations have been studied [18,45,46] and is attributed to radiative transitions from the deep oxygen-vacancy defect energy levels. It is known that In 2 O 3 , in various types of nanoformations, is a good gas (especially oxygen) absorber [47]. The In2O3 layers formed on n-InSe:Sn and p-InSe:Cd substrates are materials displaying visible photoluminescence (Figure 4a). Under laser excitation (power density 20 mW/cm 2 ) corresponding to the fundamental absorption edge of the In2O3 nanocrystallite layer on a p-InSe:Cd substrate (λ = 337.4 nm (3.68 eV)), the PL spectrum (Figure 4a, curve 1) is composed of two intense bands with maxima at 440 nm (2.75 eV) and 590 nm (2.10 eV), and a low-intensity plateau located in the wavelength range of 370-400 nm, with the edge at ~380 nm (3.22 eV).  The PL spectrum of the In 2 O 3 layer obtained by heat treatment in air, at 550 • C, for 6 h, of the undoped InSe plates (Figure 4a, curve 3) is analogous to the PL spectrum (curve 2) of the In 2 O 3 layer on an InSe:Sn substrate; it consists of a weakly asymmetric band with the maximum at 391 nm (3.17 eV). This PL band also predominates in the spectra of In 2 O 3 nanoparticle ensembles with sizes from units to tens of nanometers [30,48,49].
A narrow band with the maximum located at 388 nm is characteristic of the PL emission of the In 2 O 3 nanowire layer [48]. A PL spectrum composed of a band located in the wavelength range of 350-440 nm was also obtained for In 2 O 3 nanocubes. From the comparison of PL spectra of In 2 O 3 layers obtained by heat treatment in air, at 550 • C, for 6 h, of undoped InSe and 0.5 at.% Cd (Sn)-doped InSe plates (Figure 4), it is clear that the structure of the PL spectra is determined not only by the size and shape of nanoformations and by oxygen vacancies but also by the Cd and Sn impurities, which contribute to the luminescent recombination mechanism in In 2 O 3 . Figure 4b shows the PL spectra of undoped InSe single crystals (curve 4), InSe doped with 0.5 at.% Cd (curve 2) and Sn (curve 3), as well as the PL spectrum from the InSe:Cd/In 2 O 3 interface (curve 1), under excitation with 532 nm (2.33 eV) laser radiation with a power density of 5 mW/cm 2 . The PL spectrum of InSe crystals (curve 4) consists of a band with a weak asymmetric contour and the maximum at 1010 nm (1.28 eV), which correlates well with the optical band gap of InSe at room temperature [50]. Therefore, the PL of undoped InSe crystals is determined by the recombination of nonequilibrium charge carriers in the CB with the holes in the VB. The PL peak intensities of InSe single crystals doped with Sn and Cd are located at 1025 nm (1.210 eV) and 1047 nm (1.184 eV), respectively. These maxima exhibit a redshift, compared to the emission band of the undoped crystals, of~18 meV and 44 meV, respectively. This displacement is likely due to the shift of CB and VB edges in these crystals. The PL band, at 77 K, of Sn-doped InSe single crystals is shifted toward lower energies by 18 meV, compared to that of undoped crystals [51].
The PL spectrum of the material of the interface layer from the InSe:Cd/In 2 O 3 heterojunction (Figure 4b, curve 1) contains two bands with maxima located at 962 nm (1.287 eV) and 1003 nm (1.235 eV). These bands are shifted toward a high-energy region relative to the PL band of the primary compound (InSe:Cd) (Figure 4b, curve 2) with~100 meV and 51 meV, respectively. Such a shift can be determined by the presence of different types of nanoformations in the InSe layer from the heterojunction interface. In [52], PL spectra of InSe thin films are provided, from which a blueshift of~140 meV for film thicknesses smaller than 24 nm can be easily observed. Figure 5 shows the spectral dependencies of photoresponse (PR) (photocurrent generated per unit of incident power and unit area of detector) as a function of photon energy for the isotypic structures n-InSe:Sn/n + -In 2 O 3 (curve 1) and p-InSe:Cd/n-In 2 O 3 (curve 2). erials 2022, 15, x FOR PEER REVIEW Figure 5 shows the spectral dependencies of photoresponse generated per unit of incident power and unit area of detector) as a energy for the isotypic structures n-InSe:Sn/n + -In2O3 (curve 1) and (curve 2). The red PR threshold is determined by direct optical transition from the interface with In2O3. Since the In2O3 layer was formed by th (n)-InSe plates, the slow increase in PR together with incident photo that at the InSe:Cd/In2O3 interface, no additional recombination cen rium charge carriers are formed. The mentioned structural features group III-VI layered materials), together with high absorption coeffic mean free path of charge carriers), determine the monotonous incre sponse in heterojunctions with its native oxide (p-InSe/In2O3) and s gallium and indium monochalcogenides [53][54][55]. The abrupt drop higher than 3.65 eV (curve 2) is probably due to the absorption thr layer. Characteristic for heterojunctions formed by semiconductors o the narrow photoresponse band and the low open circuit voltage [56,5 PR of the n-InSe/n + -In2O3 structures at energies over 1.90 eV can be increase in the absorption coefficient of the n-InSe:Sn layer and by additional concentration of defects at the n-InSe/n + -In2O3 interface.
The flexibility of the n-In2O3/p-InSe:Cd heterojunction and of th resistor was studied by the repeated (cyclic) bending of the sample by curvature was determined by computational fitting of the image of th was found to be equal to ~15 cm and 12 cm for the n-In2O3/p-InSe:Cd the p-InSe:Cd photoresistor, respectively. Figure 6 shows the photoresponse in the p-InSe:Cd/n-In2O3 he the p-InSe:Cd lamellar photoresistor, depending on the number of b manufactured devices (curves 1 and 3) and for repeated measuremen The red PR threshold is determined by direct optical transitions in the InSe layer from the interface with In 2 O 3 . Since the In 2 O 3 layer was formed by the oxidation of the p (n)-InSe plates, the slow increase in PR together with incident photon energy indicates that at the InSe:Cd/In 2 O 3 interface, no additional recombination centers of nonequilibrium charge carriers are formed. The mentioned structural features of InSe (and other group III-VI layered materials), together with high absorption coefficient α ≥ 1/L (L is the mean free path of charge carriers), determine the monotonous increase in the photoresponse in heterojunctions with its native oxide (p-InSe/In 2 O 3 ) and structures based on gallium and indium monochalcogenides [53][54][55]. The abrupt drop in PR at energies higher than 3.65 eV (curve 2) is probably due to the absorption threshold of the In 2 O 3 layer. Characteristic for heterojunctions formed by semiconductors of the same type is the narrow photoresponse band and the low open circuit voltage [56,57]. The decrease in PR of the n-InSe/n + -In 2 O 3 structures at energies over 1.90 eV can be determined by the increase in the absorption coefficient of the n-InSe:Sn layer and by the presence of an additional concentration of defects at the n-InSe/n + -In 2 O 3 interface.
The flexibility of the n-In 2 O 3 /p-InSe:Cd heterojunction and of the p-InSe:Cd photoresistor was studied by the repeated (cyclic) bending of the sample by 15 • . The radius of curvature was determined by computational fitting of the image of the bent samples and was found to be equal to~15 cm and 12 cm for the n-In 2 O 3 /p-InSe:Cd heterojunction and the p-InSe:Cd photoresistor, respectively. Figure 6 shows the photoresponse in the p-InSe:Cd/n-In 2 O 3 heterojunction and in the p-InSe:Cd lamellar photoresistor, depending on the number of bends in the newly manufactured devices (curves 1 and 3) and for repeated measurements after 48 h (curves terials 2022, 15, x FOR PEER REVIEW Figure 6. Dependence of the photocurrent as a function of the number of ben for p-InSe:Cd/In2O3 heterojunctions (1, 2) and photoresistor based on the InSe:Cd plate (3, 4); curves 1 and 3 are the initial measurements; curves 2 and repeated after 48 h.
Since the dependencies of the photocurrent on the number of heterojunctions and photoresistors are similar, we can state that the fa decrease in the photocurrent in these devices are characteristic for In ously, upon bending, internal stresses are formed in the InSe layer, w change in the forbidden bandwidth and, thus, in the photoresponse b [58,59], the elastic constants and the pressure dependence of the ener lamellar compounds GaS, GaSe, and InSe were studied, from which the compressive forces between the packages are slightly decreasing from 6.28 × 10 -10 to 4.8 × 10 -10 N m −2 respectively, while the absorption toward higher energies as the pressure increases.
Consequently, one can state that bending by ~15° will exert a we PR bandwidth of the p-InSe:Cd/n-In2O3 heterojunctions. As can be s the photosensitivity band of these heterojunctions covers a broad s 1.25 to 3.70 eV. The flexible photodetectors studied in works [13,14] s ity in the UV-C region (200-300) nm.

Conclusions
By heat treatment in air, at a temperature of 600 °C, of InSe sing doped with Cd and Sn, in a water-vapor-and oxygen-enriched atmo and p (n)-InSe/n-In2O3 structures can be obtained, displaying bl broadband photosensitivity. As Raman and EDX analyses show, th formed on the surface of InSe:Sn plates is comprised of the compoun Since the dependencies of the photocurrent on the number of bending cycles for heterojunctions and photoresistors are similar, we can state that the factors leading to the decrease in the photocurrent in these devices are characteristic for InSe:Cd plates. Obviously, upon bending, internal stresses are formed in the InSe layer, which can lead to a change in the forbidden bandwidth and, thus, in the photoresponse bandwidth. In works [58,59], the elastic constants and the pressure dependence of the energy band gap in the lamellar compounds GaS, GaSe, and InSe were studied, from which it can be seen that the compressive forces between the packages are slightly decreasing from GaSe to InSe, from 6.28 × 10 −10 to 4.8 × 10 −10 N m −2 respectively, while the absorption edge slightly shifts toward higher energies as the pressure increases.
Consequently, one can state that bending by~15 • will exert a weak influence on the PR bandwidth of the p-InSe:Cd/n-In 2 O 3 heterojunctions. As can be seen from Figure 5, the photosensitivity band of these heterojunctions covers a broad spectral range, from 1.25 to 3.70 eV. The flexible photodetectors studied in works [13,14] show photosensitivity in the UV-C region (200-300) nm.

Conclusions
By heat treatment in air, at a temperature of 600 • C, of InSe single-crystalline plates doped with Cd and Sn, in a water-vapor-and oxygen-enriched atmosphere, In 2 O 3 layers and p (n)-InSe/n-In 2 O 3 structures can be obtained, displaying blue-orange PL and broadband photosensitivity. As Raman and EDX analyses show, the layer of material formed on the surface of InSe:Sn plates is comprised of the compound In 2 O 3 with an excess of absorbed oxygen.
The band gap of the native oxide layer, determined by wavelength-modulated reflectance spectroscopy, is equal to 3.57 and 3.67 eV for the In 2 O 3 layer formed by the heat treatment of single-crystalline InSe plates doped with Sn and Cd, respectively.
The In 2 O 3 layer is a photoluminescent material in the visible range. The structure of its PL spectrum is determined by actual dopants: Cd in p-InSe:Cd/n-In 2 O 3 and Sn in n-InSe:Sn/n + -In 2 O 3 structures.
The p-InSe/n-In 2 O 3 heterojunctions and p-InSe:Cd photoresistors maintain their photosensitivity upon multiple bending cycles.
The relative photosensitivity band of p-InSe/n-In 2 O 3 structures is determined by the fundamental absorption threshold of p-InSe and at higher energies, by that of In 2 O 3 .