Amorphous InGaZnO Thin-Film Transistors with Double-Stacked Channel Layers for Ultraviolet Light Detection

Amorphous InGaZnO thin film transistors (a-IGZO TFTs) with double-stacked channel layers (DSCL) were quite fit for ultraviolet (UV) light detection, where the best DSCL was prepared by the depositions of oxygen-rich (OR) IGZO followed by the oxygen-deficient (OD) IGZO films. We investigated the influences of oxygen partial pressure (PO) for DSCL-TFTs on their sensing abilities by experiments as well as Technology Computer Aided Design (TCAD) simulations. With the increase in PO values for the DSCL depositions, the sensing parameters, including photogenerated current (Iphoto), sensitivity (S), responsivity (R), and detectivity (D*) of the corresponding TFTs, apparently degraded. Compared with PO variations for the OR-IGZO films, those for the OD-IGZO depositions more strongly influenced the sensing performances of the DSCL-TFT UV light detectors. The TCAD simulations showed that the variations of the electron concentrations (or oxygen vacancy (VO) density) with PO values under UV light illuminations might account for these experimental results. Finally, some design guidelines for DSCL-TFT UV light detectors were proposed, which might benefit the potential applications of these novel semiconductor devices.


Introduction
Ultraviolet (UV) light detectors have been extensively investigated in recent years due to their wide applications in flame detection, health motoring, environmental surveillance, and optical communication [1][2][3]. Amorphous oxide semiconductors (AOSs) are interesting materials for UV light detection because of their high transparency and wide band gap (E g > 3 eV) [4][5][6]. Amorphous InGaZnO thin film transistors (a-IGZO TFTs) have especially attracted much attention as UV light detectors because of their great responsivity, small dark current, low manufacturing temperature, good uniformity, and outstanding electrical stability after bending [5][6][7][8][9][10]. In order to achieve higher UV light detectivity of a-IGZO TFTs, the researchers have reported several device improving methods, including choosing high-k gate dielectric materials, adding photosensitive absorption layers, adopting high work-function-difference capping layers, etc. [11][12][13]; on the other side, the optimization of processing conditions, e.g., using plasma enhanced atomic layer deposition (PEALD), adjusting oxygen partial pressure (P O ) during preparations, etc., also seemed effective to make a-IGZO TFTs more sensitive to UV light illuminations [14][15][16][17].
Recently, we proposed to use double-stacked channel layers (DSCL) to increase the detecting abilities of a-IGZO TFT UV sensors, resulting in a good sensitivity of 28.6 dB when they were illuminated by 370 nm UV light [18]. In contrast to the optimized DSCL structure for general-purpose TFT devices [19], the best DSCL deposition consequence of oxygen-rich (OR) IGZO followed by oxygen-deficient (OD) IGZO was proven for UV light detection [18]. However, the detailed design methods as well as the related physical essence are still unknown for a-IGZO TFTs with DSCL (DSCL-TFTs) UV light detectors.
In this study, the UV light response properties of the DSCL-TFTs using various P O were comparatively investigated, with the related physical mechanisms demonstrated through experiments as well as Technology Computer Aided Design (TCAD) simulations. It was found that the UV light photogenerated current (I photo ), sensitivity (S), responsivity (R), and detectivity (D*) of the DSCL-TFTs increased when P O for the DSCL depositions became smaller. In addition, the back channel (OD-IGZO) was more sensitive to P O variation than the front channel (OR-IGZO) under UV light illuminations. X-ray photoemission spectroscopy (XPS) and ultraviolet-visible spectrophotometer (UVS) measurements were employed to ascertain the variations of the defect density and light absorption with P O for a-IGZO depositions. Finally, a qualitative model was proposed and elaborated to explain these experimental data through TCAD simulations.

Materials and Methods
Five samples of DSCL-TFTs (Device 1-5) were prepared on the p++ silicon wafers (gate electrodes) with 500 nm-thick SiO 2 (gate insulators), with the schematic cross-section shown in the inset of Figure 1a. Among them, Device 2 was used as the reference sample. All the devices had the same structures but the processing conditions of their channel layers were different, as shown in Table 1. Both the OD-IGZO and OR-IGZO were deposited via magnetron sputtering, where the atomic ratio of the target was In: Ga: Zn = 1:1:1. After the DSCL depositions, the 200 nm-thick indium tin oxide (ITO) layers were prepared as source/drain (S/D) electrodes, followed by the 50 nm-thick SiO 2 layers as passivation layers. Both the S/D electrodes and the passivation layers were also deposited by magnetron sputtering. Three shadow masks were used to pattern the DSCL, S/D electrodes, and passivation layers during sputtering, leading to the channel width/length of 1000 µm/275 µm, respectively. Finally, all the samples were annealed at 425 • C in N 2 for 7200 s. detection [18]. However, the detailed design methods as well as the related physical essence are still unknown for a-IGZO TFTs with DSCL (DSCL-TFTs) UV light detectors. In this study, the UV light response properties of the DSCL-TFTs using various PO were comparatively investigated, with the related physical mechanisms demonstrated through experiments as well as Technology Computer Aided Design (TCAD) simulations. It was found that the UV light photogenerated current (Iphoto), sensitivity (S), responsivity (R), and detectivity (D*) of the DSCL-TFTs increased when PO for the DSCL depositions became smaller. In addition, the back channel (OD-IGZO) was more sensitive to PO variation than the front channel (OR-IGZO) under UV light illuminations. X-ray photoemission spectroscopy (XPS) and ultraviolet-visible spectrophotometer (UVS) measurements were employed to ascertain the variations of the defect density and light absorption with PO for a-IGZO depositions. Finally, a qualitative model was proposed and elaborated to explain these experimental data through TCAD simulations.

Materials and Methods
Five samples of DSCL-TFTs (Device 1-5) were prepared on the p++ silicon wafers (gate electrodes) with 500 nm-thick SiO2 (gate insulators), with the schematic cross-section shown in the inset of Figure 1a. Among them, Device 2 was used as the reference sample. All the devices had the same structures but the processing conditions of their channel layers were different, as shown in Table 1. Both the OD-IGZO and OR-IGZO were deposited via magnetron sputtering, where the atomic ratio of the target was In: Ga: Zn = 1:1:1. After the DSCL depositions, the 200 nm-thick indium tin oxide (ITO) layers were prepared as source/drain (S/D) electrodes, followed by the 50 nm-thick SiO2 layers as passivation layers. Both the S/D electrodes and the passivation layers were also deposited by magnetron sputtering. Three shadow masks were used to pattern the DSCL, S/D electrodes, and passivation layers during sputtering, leading to the channel width/length of 1000 μm/275 μm, respectively. Finally, all the samples were annealed at 425 °C in N2 for 7200 s.  The electrical properties of the DSCL-TFTs were measured at room temperature (RT) using a Keithley 2636 semiconductor parameter analyzer (Solon, OH, USA). The 380 nm UV light illumination was achieved by the combination of a 150 W Xenon lamp, a monochromator, and an optical fiber. The incident optical power density was measured by an optical power meter (Thorlabs, PM100A, Newton, NJ, USA) with a Si photodiode sensor  The electrical properties of the DSCL-TFTs were measured at room temperature (RT) using a Keithley 2636 semiconductor parameter analyzer (Solon, OH, USA). The 380 nm UV light illumination was achieved by the combination of a 150 W Xenon lamp, a monochromator, and an optical fiber. The incident optical power density was measured by an optical power meter (Thorlabs, PM100A, Newton, NJ, USA) with a Si photodiode sensor (Thorlabs, S120VC, Newton, NJ, USA), which was confirmed as 0.085 mW/cm 2 . The transmittance and the chemical bonding states of a-IGZO films were measured by a UV-visible spectrophotometer (EVOLUTION 300, Waltham, MA, USA) and an XPS analyzer (AXIS Ultra DLD, Manchester, UK), respectively. In order to thoroughly clean the sample surfaces, 10 nm-depth Ar-ion etching treatments were employed before recording the XPS spectra. Victory Device, one of the most popular TCAD tools from Silvaco, Inc., (Santa Clara, CA, USA) was used to investigate the physical essence relating the experimental results reported in this study [20]. Figure 1a shows the transfer characteristics of the five samples. One may notice that the transfer curves of the DSCL-TFTs shifted positively with P O (for the channellayer depositions) increasing which is consistent with other reports [21]. Interestingly, these curves were quite sensitive to the UV light illuminations. As shown in Figure 1b, the transfer curve of Device 1 apparently shifted in the negative direction when it was illuminated by the 380 nm UV light for 600 s. However, this sensitivity to the UV light illumination was different for the five samples, implying that the P O values for the DSCL depositions evidently influenced the defect density in a-IGZO under UV light illuminations.

Results and Discussion
In order to quantitatively study the sensing properties of the DSCL-TFTs, we defined some useful terms, i.e., net photogenerated current (I photo ), sensitivity (S), responsivity (R), and detectivity (D*) [4,18]. I photo was defined as follows: where I illuminated is the total photo current under illumination and I dark is the dark current.
In this study, I dark was fixed as 10 −10 A for all the measurements and I illuminated was obtained under the same gate voltage corresponding to I dark . Sensitivity (S), the ratio of the net photogenerated current and the dark current of the photodetectors, was defined as follows: Responsivity (R), the ratio of the net photogenerated current and the incident light power of the photodetectors, was defined as follows: where P light is the incident light power. Detectivity (D*), a figure about the minimum detection of photodetectors, which was considered as the normalization of responsivity [16], was defined as follows: where e is elementary charge and J dark is the dark current density. Figure 2a,b demonstrates the dependence of I photo , S, R, and D* on P O for the OD-IGZO depositions. Here, the P O values for OD-IGZO increased from 0 mPa to 14 mPa, while P O for OR-IGZO was fixed at 21 mPa. On the other hand, Figure 2c,d shows the influence of P O for the OR-IGZO depositions on I photo , S, R, and D*. Here, the P O values for OR-IGZO increased from 21 mPa to 56 mPa, while P O for OD-IGZO was fixed at 7 mPa. Obviously, all these parameters, including I photo , S, R, and D*, decreased with P O increasing. In addition, for the purpose of analyzing the UV light sensing degradation of the DSCL-TFTs with the increase in P O values, the variation ratio ∆I photo /∆P O was defined in this study (see Table 2). For the case of the P O variation for OD-IGZO, ∆I photo /∆P O was −7.5 × 10 −11 A·mPa −1 . However, when the P O value for OR-IGZO changed, ∆I photo /∆P O became −1.9 × 10 −11 A·mPa −1 . Similarly, when P O for OD-IGZO increased, ∆S/∆P O , ∆R/∆P O , and ∆D*/∆P O were −1.9 dB·mPa −1 , −3.2 × 10 −4 A·W −1 ·mPa −1 , and −2.2 × 10 9 Jones·mPa −1 , respectively. However, when P O for OR-IGZO increased, ∆S/∆P O , ∆R/∆P O , and ∆D*/∆P O were −0.8 dB·mPa −1 , −8.2 × 10 −5 A·W −1 ·mPa −1 , and −5.6 × 10 8 Jones·mPa −1 , respectively. We may draw a conclusion that the UV light response properties of the DSCL-TFTs were more sensitive to P O variations for the back channel (OD-IGZO) than those for the front channel (OR-IGZO). These results are consistent with a recent publication, which indicated that the oxygen vacancies (V O ) located at the back channel of the a-IGZO layer played an important role in UV light response [22]. This conclusion might lead to some new approaches to improving the DSCL-TFT UV light detectors by the modulation of P O valves. × 10 −11 A•mPa −1 . However, when the PO value for OR-IGZO changed, ΔIphoto/ΔPO became −1.9 × 10 −11 A•mPa −1 . Similarly, when PO for OD-IGZO increased, ΔS/ΔPO, ΔR/ΔPO, and ΔD*/ΔPO were −1.9 dB•mPa −1 , −3.2 × 10 −4 A•W −1 •mPa −1 , and −2.2 × 10 9 Jones•mPa −1 , respectively. However, when PO for OR-IGZO increased, ΔS/ΔPO, ΔR/ΔPO, and ΔD*/ΔPO were −0.8 dB•mPa −1 , −8.2 × 10 −5 A•W −1 •mPa −1 , and −5.6 × 10 8 Jones•mPa −1 , respectively. We may draw a conclusion that the UV light response properties of the DSCL-TFTs were more sensitive to PO variations for the back channel (OD-IGZO) than those for the front channel (OR-IGZO). These results are consistent with a recent publication, which indicated that the oxygen vacancies (VO) located at the back channel of the a-IGZO layer played an important role in UV light response [22]. This conclusion might lead to some new approaches to improving the DSCL-TFT UV light detectors by the modulation of PO valves.
To analyze the physical essence relating the abovementioned experimental results, we used a UV-visible spectrophotometer and an XPS analyzer to characterize the differences between the material properties of OD-IGZO and OR-IGZO. Figure 3 illustrates the transmittance spectra of OD-IGZO and OR-IGZO films, the corresponding Tauc plots, and linear fitting lines, which are shown in the insets. After obtaining the adsorption spectra from the transmittance spectra, we derived the optical energy band gaps by Tauc law using the following equation [19]: Here, 1 Jones = 1 cm·Hz 0.5 ·W −1 .
To analyze the physical essence relating the abovementioned experimental results, we used a UV-visible spectrophotometer and an XPS analyzer to characterize the differences between the material properties of OD-IGZO and OR-IGZO. Figure 3 illustrates the transmittance spectra of OD-IGZO and OR-IGZO films, the corresponding Tauc plots, and linear fitting lines, which are shown in the insets. After obtaining the adsorption spectra from the transmittance spectra, we derived the optical energy band gaps by Tauc law using the following equation [19]: where α is the absorption coefficient, h is the Planck constant, hυ represents the photon energy, and A is a constant related to UV light adsorption. The value of E g was determined by the intersection point of the linear fitting line and the x-axis. The overall transmittances of all the a-IGZO films were larger than 90% in the visible light region, though they quickly dropped when the light wavelength decreased below 400 nm, confirming the good UV light adsorption of a-IGZO films. As shown in Figure 3, both OD-IGZO and OR-IGZO exhibited almost the same optical bandgap values, i.e., around 3.7 eV. This suggests that P O for a-IGZO depositions hardly influenced the UV light absorption of a-IGZO films in this study.
where α is the absorption coefficient, h is the Planck constant, hυ represents the photon energy, and A is a constant related to UV light adsorption. The value of Eg was determined by the intersection point of the linear fitting line and the x-axis. The overall transmittances of all the a-IGZO films were larger than 90% in the visible light region, though they quickly dropped when the light wavelength decreased below 400 nm, confirming the good UV light adsorption of a-IGZO films. As shown in Figure 3, both OD-IGZO and OR-IGZO exhibited almost the same optical bandgap values, i.e., around 3.7 eV. This suggests that PO for a-IGZO depositions hardly influenced the UV light absorption of a-IGZO films in this study.   Figure 1. All the O1s spectra were calibrated by using the C1s (284.8 eV) as the reference [23][24][25][26], where the O1s peak was deconvoluted into three Gaussian fitting sub-peaks that approximately centered at 530.3 eV (OI), 531.0 eV (OII), and 532.2 eV (OIII), respectively. The low binding energy OI peak could be attributed to the oxygen bonds with metal, the high binding energy OIII peak might be related to the hydrated oxides defects, and the middle binding energy OII peak was associated with oxygen vacancies (VO) [26]. In order to characterize the variations of VO with the PO values for IGZO deposition, the peak area ratio of the OII over the total area of O1s peak (OTotal = OI + OII + OIII) was calculated. One may notice that the area ratio OII/OTotal decreased from 20.7% to 10.8% when PO increased from 0 mPa to 56 mPa. These results proved that the VO density of the a-IGZO layer evidently decreased with PO increasing during its deposition.   Figure 1. All the O1s spectra were calibrated by using the C1s (284.8 eV) as the reference [23][24][25][26], where the O1s peak was deconvoluted into three Gaussian fitting sub-peaks that approximately centered at 530.3 eV (O I ), 531.0 eV (O II ), and 532.2 eV (O III ), respectively. The low binding energy O I peak could be attributed to the oxygen bonds with metal, the high binding energy O III peak might be related to the hydrated oxides defects, and the middle binding energy O II peak was associated with oxygen vacancies (V O ) [26]. In order to characterize the variations of V O with the P O values for IGZO deposition, the peak area ratio of the O II over the total area of O1s peak (O Total = O I + O II + O III ) was calculated. One may notice that the area ratio O II /O Total decreased from 20.7% to 10.8% when P O increased from 0 mPa to 56 mPa. These results proved that the V O density of the a-IGZO layer evidently decreased with P O increasing during its deposition.
So far, three important results have been obtained from the aforementioned experiments: (1) The UV light response properties of the DSCL-TFTs evidently depended on the P O value for the channel layer depositions; (2) The P O variation for OD-IGZO at the top side of DSCL showed stronger influences on DSCL-TFT UV detectors than that for OR-IGZO at the bottom side of DSCL; (3) P O hardly influenced the UV light absorption of a-IGZO films but evidently changed the defect density, especially the Vo density. To ascertain the related physical mechanisms, we employed TCAD simulations and analysis on the DSCL-TFTs illuminated by UV lights. Exponential and Gaussian functions were used to model the band tail states and deep states in a-IGZO films, respectively. Specifically, the donor-like tail states (g TD ), the acceptor-like tail states (g TA ), the donor-like deep states (g GD ), and the acceptor-like deep states (g GA ) were defined as Equations (6)-(9) [20]. Here, E c and E v is the conduction band edge energy and the valence band edge energy, respectively. The exact meanings of the corresponding parameters are all listed in Table 3. Micromachines 2022, 13, x FOR PEER REVIEW 6 of 11 So far, three important results have been obtained from the aforementioned experiments: (1) The UV light response properties of the DSCL-TFTs evidently depended on the PO value for the channel layer depositions; (2) The PO variation for OD-IGZO at the top side of DSCL showed stronger influences on DSCL-TFT UV detectors than that for OR-IGZO at the bottom side of DSCL; (3) PO hardly influenced the UV light absorption of a-IGZO films but evidently changed the defect density, especially the Vo density. To ascertain the related physical mechanisms, we employed TCAD simulations and analysis on the DSCL-TFTs illuminated by UV lights. Exponential and Gaussian functions were used to model the band tail states and deep states in a-IGZO films, respectively. Specifically, the donor-like tail states (gTD), the acceptor-like tail states (gTA), the donor-like deep states (gGD), and the acceptor-like deep states (gGA) were defined as Equations (6)-(9) [20]. Here, Ec and Ev is the conduction band edge energy and the valence band edge energy, respectively. The exact meanings of the corresponding parameters are all listed in Table 3.   As shown in Table 3, n(V O ) is the initial Vo concentration and n(V O 2+ ) represents the initial secondary ionized V O concentration. For the simulations, there were two reactions to describe the ionization process in a-IGZO [20]: Here, V x O and V •• O represent neutral oxygen vacancy and secondary ionized oxygen vacancy, respectively. Reaction (10) indicates that n(V O 2+ ) should be affected by n(V O ), which is related to P O for a-IGZO deposition. Accordingly, n(V O 2+ ) is indirectly influenced by the P O value. It is generally believed that NGD is mainly associated with the V O density [19,21]. Therefore, n(V O ), n(V O 2+ ), and NGD are all connected to the P O values for a-IGZO depositions. Figure 5a shows the fitting results between the simulation data and the experimental transfer curve. With the typical parameters listed in Table 3 and the device built in the inset of Figure 5a, the simulated transfer curve of the DSCL-TFTs agreed well with the experimental data, suggesting that our TCAD model could be used to investigate the physical essence relating the experiments employed in this study. The distribution of the electron concentration (n e ) in DSCL is exhibited in Figure 5b when V gs = 0 V. Figure 5b shows the detailed simulation results about the area highlighted by a red arrow in the inset of Figure 5a. One may observe that the electron concentration gradually decreased from the back channel to the front channel, where the n e values at the back channel and the front channel were 1 × 10 14 cm −3 and 1 × 10 13 cm −3 , respectively. This was consistent with the XPS characterization results shown in Figure 4.  After the DSCL-TFTs were illuminated by the 380 nm UV light for 600 s, the electron concentration ne increased to neʹ. The variation of the electron concentration (Δne = neʹ−ne) could microscopically denote the UV light sensing abilities of the DSCL-TFTs. Apparently, the larger the Δne value, the more sensitive the sample. As shown in Figure 6, Δne of the reference sample gradually decreased from the back channel to the front channel. The simulation studies exhibited that Δne apparently decreased by increasing PO either for OD-IGZO (as shown in Figure 6a) or for OR-IGZO (as shown in Figure 6b). This result explained the experimental results shown in Figure 2, i.e., the UV light sensing abilities of the DSCL-TFTs became worse with PO increasing. On the other side, the PO modulation effects from the OD-IGZO and OR-IGZO were different. From the aforementioned experiments, the PO variation for OD-IGZO deposition showed stronger influence than that for OR-IGZO. To more deeply explore this difference, we calculated the total Δne by summing all the data points shown in Figure 6a,b. As shown in Table 4, the increase in PO for OD-IGZO showed stronger influences on the total Δne than that for OR-IGZO, which is also consistent with the measurement results shown in Figure 2. It is well known that the electron concentration closely relates oxygen vacancies and the other defects in a-IGZO [27,28], so the simulation results shown in Figure 6 also reflected how the defects (espe- After the DSCL-TFTs were illuminated by the 380 nm UV light for 600 s, the electron concentration n e increased to n e . The variation of the electron concentration (∆n e = n e − n e ) could microscopically denote the UV light sensing abilities of the DSCL-TFTs. Apparently, the larger the ∆n e value, the more sensitive the sample. As shown in Figure 6, ∆n e of the reference sample gradually decreased from the back channel to the front channel. The simulation studies exhibited that ∆n e apparently decreased by increasing P O either for OD-IGZO (as shown in Figure 6a) or for OR-IGZO (as shown in Figure 6b). This result explained the experimental results shown in Figure 2, i.e., the UV light sensing abilities of the DSCL-TFTs became worse with P O increasing. On the other side, the P O modulation effects from the OD-IGZO and OR-IGZO were different. From the aforementioned experiments, the P O variation for OD-IGZO deposition showed stronger influence than that for OR-IGZO. To more deeply explore this difference, we calculated the total ∆n e by summing all the data points shown in Figure 6a,b. As shown in Table 4, the increase in P O for OD-IGZO showed stronger influences on the total ∆n e than that for OR-IGZO, which is also consistent with the measurement results shown in Figure 2. It is well known that the electron concentration closely relates oxygen vacancies and the other defects in a-IGZO [27,28], so the simulation results shown in Figure 6 also reflected how the defects (especially V O ) changed with P O and UV light illuminations. Therefore, for DSCL-TFT UV light detectors, the defects in OD-IGZO (especially the V O density) were more easily modulated by P O than those in OR-IGZO.  According to all the experimental data and simulation results, we made a deeper discussion on the PO effect for DSCL-TFT UV light response. From the UVS characterization results shown in Figure 3, we could assume that band-to-band electron excitation would be nearly the same for all the devices in this study. On the one hand, the net photogenerated electron concentration (Δne) decreased with PO for DSCL increasing and the photogenerated VO 2+ were believed to play an important role in UV light sensing [22,28]. Therefore, we could suppose that the PO increase during the DSCL depositions might reduce the concentration of photogenerated VO 2+ and result in smaller Δne in the channel layers. There are two main photogenerated VO creation mechanisms under the UV light illuminations, which could be formed by using the energy released from electron-hole recombination or photogenerated owing to the high energy photons [22]. Therefore, the concentration of photogenerated VO 2+ might decrease when PO for a-IGZO depositions increased; this might be induced by lower photoionization of VO to VO 2+ rather than lower VO creation under the illumination, because the photogenerated VO might hardly be affected by the PO value for a-IGZO. In other words, when the PO value for a-IGZO deposition increased, VO 2+ from the photoionization of VO decreased, resulting in a decrease in Δne and thus less UV light sensing for the DSCL-TFTs.
Finally, we may reach some design guidelines for DSCL-TFT UV detectors: (1) The DSCL consisting of an OD-IGZO (top side) and an OR-IGZO (bottom side) is the best choice for UV light detection; (2) For the deposition of DSCL, lower oxygen partial pressures are preferred; (3) To modulate the UV light sensing abilities of DSCL-TFTs, the OD-IGZO, rather than OR-IGZO, is more sensitive to variations in PO values.

Conclusions
The influences of oxygen partial pressures for DSCL-TFTs on their UV light sensing abilities were investigated by both experimental studies and TCAD simulations. With the  According to all the experimental data and simulation results, we made a deeper discussion on the P O effect for DSCL-TFT UV light response. From the UVS characterization results shown in Figure 3, we could assume that band-to-band electron excitation would be nearly the same for all the devices in this study. On the one hand, the net photogenerated electron concentration (∆n e ) decreased with P O for DSCL increasing and the photogenerated V O 2+ were believed to play an important role in UV light sensing [22,28]. Therefore, we could suppose that the P O increase during the DSCL depositions might reduce the concentration of photogenerated V O 2+ and result in smaller ∆n e in the channel layers. There are two main photogenerated V O creation mechanisms under the UV light illuminations, which could be formed by using the energy released from electron-hole recombination or photogenerated owing to the high energy photons [22]. Therefore, the concentration of photogenerated V O 2+ might decrease when P O for a-IGZO depositions increased; this might be induced by lower photoionization of V O to V O 2+ rather than lower V O creation under the illumination, because the photogenerated V O might hardly be affected by the P O value for a-IGZO. In other words, when the P O value for a-IGZO deposition increased, V O 2+ from the photoionization of V O decreased, resulting in a decrease in ∆n e and thus less UV light sensing for the DSCL-TFTs.
Finally, we may reach some design guidelines for DSCL-TFT UV detectors: (1) The DSCL consisting of an OD-IGZO (top side) and an OR-IGZO (bottom side) is the best choice for UV light detection; (2) For the deposition of DSCL, lower oxygen partial pressures are preferred; (3) To modulate the UV light sensing abilities of DSCL-TFTs, the OD-IGZO, rather than OR-IGZO, is more sensitive to variations in P O values.

Conclusions
The influences of oxygen partial pressures for DSCL-TFTs on their UV light sensing abilities were investigated by both experimental studies and TCAD simulations. With the increase in P O values for the DSCL depositions, the sensing parameters, including I photo , S, R, and D* of the corresponding TFTs, apparently became worse. Compared with the P O variations for the OR-IGZO films, those for the OD-IGZO depositions showed stronger influences on the sensing performances of the DSCL-TFT UV light detectors. The TCAD simulations indicated that the variations of the electron concentrations (or the V O density) with P O values under UV light illuminations should be responsible for the aforementioned experimental results. Some design guidelines for DSCL-TFT UV light detectors were finally proposed for the potential applications of these novel semiconductor devices.

Data Availability Statement:
The data presented in this study are available on request from the corresponding author.