Vishnu
Aggarwal
abc,
Manish
Kumar
d,
Rahul
Kumar
ab,
Sudhanshu
Gautam
ab,
Aditya
Yadav
ab,
Shikha
Shrivastava
ab,
Anjana
Dogra
ab,
Govind
Gupta
ab,
Sumeet
Walia
c and
Sunil Singh
Kushvaha
*ab
aCSIR-National Physical Laboratory, Dr K. S. Krishnan Road, New Delhi 110012, India. E-mail: kushvahas@nplindia.org
bAcademy of Scientific and Innovative Research (AcSIR), Ghaziabad 201002, India
cSchool of Engineering, RMIT University, Melbourne, Victoria 3000, Australia
dPhysics Department and CSMB, Humboldt-Universität zu Berlin, Zum Großen Windkanal 2, 12489 Berlin, Germany
First published on 12th November 2024
For practical optoelectronic applications, photodetectors capable of detecting light across a wide wavelength range (200–1100 nm) are essential. Heterojunction semiconductors play a crucial role in developing such multi-wavelength photodetectors. In particular, the heterojunction of transition metal chalcogenides (tuneable bandgap and high electron mobility) and Ga2O3 (wide bandgap of >4 eV) is a significant research topic for photodetector fabrication exhibiting an ultrawide spectral photodetection capability. In this study, epitaxial β-Ga2O3 thin films were grown on atomically flat sapphire (0001) and p-GaN/sapphire (0001) surfaces using a pulsed laser deposition technique. The effect of the substrate on the crystalline, optical, electronic, and photoresponse properties of β-Ga2O3 thin films was thoroughly investigated and correlated with theoretical insights from density functional theory. To achieve broadband photodetection, a heterojunction of MoSe2 and the as-grown Ga2O3 films was fabricated, enabling light detection from the deep ultraviolet (UV) to the near-infrared (NIR) spectral regions. The MoSe2/Ga2O3/p-GaN device exhibited an expanded detection range from deep ultraviolet (240–320 nm) to long-wavelength ultraviolet (320–400 nm) and a significant responsivity of 5.5 A W−1 in the NIR region, nearly fourfold higher than that of the MoSe2/Ga2O3/sapphire device. These results highlight the potential of these hybrid structures for developing multi-wavelength photodetectors with high photoresponse across the deep-UV to NIR spectral regions, offering promising applications in fields ranging from environmental monitoring to communications.
In contrast, Ga2O3 is an ideal choice for DUV PDs due to its direct and UWBG of 4.4–5.0 eV, high breakdown electric field (theoretical value ∼8 MV cm−1), chemical robustness, and radiation hardness.6,13–15 The n-type semiconductor properties in Ga2O3 primarily arise from intrinsic oxygen deficiencies. However, creating a p–n homojunction in Ga2O3 is challenging due to the difficulty in achieving p-type doping.13–15 To fully harness the potential of β-Ga2O3, an alternative approach involves creating p–n heterojunctions by integrating Ga2O3 with other p-type wide-bandgap (WBG) semiconductors, such as SiC, GaN, NiO, and CuSCN. Integrating these WBG semiconductors with Ga2O3 not only enhances the photodetection properties of Ga2O3-based photodetectors but also expands the wavelength range of UV photodetection.16–19 Among these semiconductors, GaN stands out as a promising candidate for integration with Ga2O3 to develop highly efficient solar-blind photodetectors. This is due to the low lattice mismatch between the (002) plane of GaN and the (−201) plane of Ga2O3, along with GaN's superior physical properties, such as its direct bandgap of 3.4 eV, a low excitonic binding energy of approximately 25 meV, and high electron mobility.20,21 Furthermore, in recent years, van der Waals (vdW) heterojunctions have gained significant attention due to their exceptional properties, including enhanced conductivity, wide-spectrum light absorption, and high carrier mobility.22–25 Furthermore, the vdW heterojunction of Ga2O3 with two-dimensional (2D) transition metal dichalcogenides (TMDs) semiconductors is a significant research topic for photodetector fabrication exhibiting broad spectral photoresponse capability.26,27 However, the vdW heterojunction of MoS2 and Ga2O3 has mostly been explored. In contrast, superior carrier mobility and a narrower band gap of MoSe2 than MoS2 can be advantageous for ultrawide photodetection, including visible to near-infra-red (NIR) regions.28,29
In this study, we have systematically investigated the photoresponse capability of single and dual junction photodetectors for ultrawide spectral photodetection (p–n junction: n-Ga2O3/p-GaN and vdW heterojunction: MoSe2/Ga2O3). Ga2O3 was grown on pristine sapphire (0001) and p-GaN/sapphire at 750 °C using the pulsed laser deposition (PLD) technique. High-resolution X-ray diffraction (HRXRD) 2θ–ω scans confirmed the formation of the β-phase of Ga2O3 on both substrates. Furthermore, the crystalline, structural, optical, and electronic properties of PLD grown β-Ga2O3 are elucidated, and outcomes are correlated with theoretical study via density functional theory (DFT) calculations. The photoresponse study of as-grown Ga2O3 was performed by fabricating metal–semiconductor–metal (MSM) type photodetector devices. Furthermore, a magnetron-sputtered MoSe2 thin film was decorated with Ga2O3/sapphire and Ga2O3/p-GaN/sapphire to explore the photoresponse properties of single and dual junction photodetectors. The resulting dual junction MoSe2-decorated Ga2O3/p-GaN photodetector demonstrated significantly higher responsivity compared to the single junction, with values of 32.7, 25.2, and 5.5 A W−1 in the deep-UV (UV-C), UV-A, and NIR regions at an applied voltage of 10 V.
Fig. 1(a) displays the HRXRD 2θ − ω scan results for the GS and GT samples in the 2θ range of 10 to 90°. The diffraction peaks for the GS sample were observed at positions of 18.90, 38.30, and 58.90°, corresponding to the (−201), (−402), and (−603) planes of Ga2O3, respectively.37 Similarly, the XRD peaks for Ga2O3 in the GT sample were located at 2θ angles of 18.82, 38.20, and 58.94°, related to its (−201), (−402), and (−603) Ga2O3 crystal planes.37–39 The XRD diffraction peaks are indexed using the JCPDS file 41–1103. It is clear from the 2θ − ω scan that the PLD-grown Ga2O3 has been grown in only one direction-oriented plane {−2n0n}, which indicates the formation of the β-Ga2O3 phase. It was determined that the oxygen arrangement on sapphire (0001) is equivalent to that on β-Ga2O3 (−201). As a result, this orientation is preferred.40 The higher intensity and lower full width at half maximum (FWHM) of the Ga2O3 XRD peaks in the GT sample compared with those of the GS sample reveal the better crystalline quality of the GT sample.37 Further, the peak at 41.2° in the 2θ − ω scan of both the GS and GT samples is related to the (0006) plane of the sapphire substrate. The additional peaks present in the 2θ − ω scan of the GT sample at 34.46 and 72.62° correspond to the (0002) and (0004) planes of GaN, respectively.41
Fig. 1 (a) HR-XRD 2θ–ω scan and (b) Raman spectra of the GS (Ga2O3/sapphire) and GT (Ga2O3/p-GaN/sapphire) samples. (c) and (d) Fitted PL spectra of the GS and GT samples, respectively. |
Furthermore, to analyze the structural properties of PLD-grown Ga2O3, we performed Raman spectroscopic measurements ranging from 150 to 800 cm−1, as shown in Fig. 1(b). The inset of Fig. 1(b) presents the magnified view of the Raman spectra of the GS and GT samples in the range of 150 to 400 cm−1. The Raman spectrum in the inset reveals that the Raman peaks of the GS sample are located at Raman shifts of 171.4, 201.0, and 346.9 cm−1 and are attributed to the A(2)g, A(3)g, and A(5)g characteristic phonon modes of Ga2O3, respectively, while the characteristic Raman peaks of Ga2O3 in the GT sample are located at 170.1, 201.1, and 348.9 cm−1.42,43 Furthermore, the peaks marked by an asterisk are related to the sapphire substrate.42,43 In contrast, the additional peaks in the Raman spectrum of the GT sample are the characteristic phonon modes of GaN identified as E2 (high), A1 (TO), and A1 (LO).44 The intensity of the Raman peaks of the GT sample was higher than that of the GS sample peaks, which reveals its better structural quality than that of the GS sample.
Next, we performed PL spectroscopy measurements to study the optical properties of the PLD-grown Ga2O3 samples. Fig. 1(c) and (d) show the PL spectra in the 240 to 800 nm wavelength region of the PLD-grown Ga2O3 samples. Fig. 1(c) shows the PL spectrum of the GS sample, which determines the near band edge emission of Ga2O3 at a wavelength of 266 nm, which indicates that the optical band gap of the PLD-grown Ga2O3 on sapphire is ∼4.6 eV.31 Similarly, the PL spectra of the GT sample are shown in Fig. 1(d), where the NBE emission of Ga2O3 occurred at 266 nm, revealing its band gap to be ∼4.6 eV. The quenching of the NBE peak intensity in the GT sample indicates reduced electron–hole overlap/recombination, confirming efficient charge carrier separation at the heterojunction interface.31,45 Furthermore, defect-related overlapping peaks were observed in the PL spectrum of both Ga2O3 samples, deconvoluted using the Gaussian function. The PL emission peaks in the range from 400 to 650 nm are attributed to the recombination of electrons and holes trapped in an acceptor and donor band, which originates due to oxygen and gallium vacancies, respectively, and the emission band beyond 650 nm is due to self-trapped defects. These defects are considered the primary cause of the persistent photoconductance (PPC) effect in oxide-based PDs.46–48 It was depicted from the deconvoluted peaks in the overlapped defect band that the area under the donor–acceptor pair (DAP) transition and self-trapped defects was estimated to be smaller in the GT sample compared to the GS sample. The lower intensity of the NBE peak and the lower area under the defect-related peaks in the GT sample convey its better quality than the GS sample. In addition, PL spectroscopy of the p-GaN template was performed, and the Voigt function fitted PL spectrum is shown in Fig. S2(a) (ESI†). The schematic of the energy band diagram for various transitions of electrons in the p-GaN template is shown in Fig. S2(b) (ESI†).
To study the chemical composition and valence states of elements on the surface of PLD-grown Ga2O3 films, we have performed an XPS core level scan on both samples, as shown in Fig. 2. The core level scan was deconvoluted using a mixed type of Gaussian–Lorentzian (Voigt) function, and the background was fitted using Sherley-type fitting. The core level Ga 3d spectrum of the GS sample is shown in Fig. 2(a) in the binding energy range of 17 to 27 eV. The Ga 3d spectrum is deconvoluted into three peaks at 20.19 eV, 20.92 eV, and 23.65 eV. The deconvoluted high-intensity peak at a binding energy of 20.92 eV is related to the Ga3+ chemical state, indicating a Ga–O bond associated with Ga2O3.49,50 In comparison, a low-intensity peak at 20.19 eV reveals the presence of a Ga2+ chemical state due to its location in between the Ga3+ and Ga+ chemical states, whose binding energy lies at 20.3 eV and 19.3 eV.49 In addition, a broad peak can be seen centered around the binding energy of 23.65 eV, which corresponds to the O 2s.49,50 Furthermore, Fig. 2(b) shows that the O 1s scan was performed to analyze the oxygen binding states on the surface of PLD-grown Ga2O3/sapphire. The XPS O 1s core level spectrum was deconvoluted into two peaks: the peak centered at 531.49 eV is assigned to lattice oxygen with the O2− chemical state associated with the metal–oxide bond, i.e., in Ga2O3 while the peak at 531.77 eV corresponds to oxygen vacant bonds (OV), specifically residual hydroxide species coupling with oxygen vacancies in Ga2O3.47,49–51 Similarly, the Ga 3d core level spectrum of the GT sample has been fitted to three peaks at binding energies of 17.84 eV, 19.28 eV, and 22.02 eV, corresponding to Ga2+, Ga3+ and O 2s chemical states, respectively, as shown in Fig. 2(c). Here also, the Ga3+ state and Ga2+ state indicate the formation of Ga–O bonds associated with Ga2O3 and GaO at the surface of Ga2O3 grown on p-GaN/sapphire (0001) using the PLD technique.49,50 Furthermore, the XPS O 1s core level spectrum was analyzed by fitting it to two peaks [Fig. 2(d)]. The first peak, centered at 529.84 eV, is attributed to lattice oxygen with an O2− chemical state associated with the metal–oxide bond in Ga2O3, and the second peak at 531.51 eV corresponds to oxygen vacant bonds, specifically residual hydroxide species coupling with oxygen vacancies in Ga2O3.47,49–51 It was observed that the binding energy difference of Ga3+ and O2− remained the same for both samples, which is 510.57 eV. In addition, two types of changes were observed in the XPS core-level scans of the GT sample when fitted with the same set of parameters as in core-level scans of the GS sample, except for the area of peaks, without introducing any additional component. First, the Ga2O3 component in the GT sample is likely higher than that of the GS sample as the relative ratio of the Ga3+ peak in the GT sample was estimated to be 85.39% compared to 78.25% in the GS sample [Table 1].
Fig. 2 XPS core level Ga 3d and O 1s scans of the (a) and (b) GS and (c) and (d) GT samples, and valence band spectra for the valence band maxima calculation of the (e) GS and (f) GT samples. |
XPS core level scan | Deconvoluted constituents | GS sample | GT sample | ||||
---|---|---|---|---|---|---|---|
Binding energy (eV) | FWHM (eV) | Relative % | Binding energy (eV) | FWHM (eV) | Relative % | ||
Ga 3d | Ga2+ | 20.20 | 2.19 | 16.72 | 17.83 | 1.39 | 7.20 |
Ga3+ | 20.92 | 1.46 | 78.25 | 19.28 | 1.46 | 85.39 | |
O 2s | 23.65 | 3.03 | 5.01 | 22.03 | 3.01 | 7.40 | |
O 1s | O2− | 531.49 | 1.47 | 80.36 | 529.84 | 1.47 | 91.02 |
Ov | 531.77 | 2.53 | 19.63 | 531.51 | 1.48 | 8.97 | |
E VBM | — | 3.74 eV | 2.31 eV |
Second, the binding energy of both Ga3+ and O2− peaks was lower than that of the GS sample, with a difference in the binding energy of 1.64 eV. The binding energy shift towards lower energy in the GT sample compared to the GS sample indicates that surface band bending (SBB) occurred in the GT sample with the introduction of p-GaN.52 Additionally, the different energy shifts in the binding energy of the components of the O 1s core level scan (O2− and OV) were observed in both samples, which indicated the inhomogeneous SBB in the GT sample. Furthermore, the N 1s core level scans for the pristine p-GaN template and after the growth of Ga2O3 onto the p-GaN template, i.e., the GT sample, are shown in Fig. S2(c) and (d) (ESI†) respectively. It can be noticed in Fig. S2(d) (ESI†), that the Auger signals diminished after the growth of Ga2O3. To further confirm the effect of SBB, we performed valence band spectra measurements on both the GS and GT samples. Fig. S2(e) (ESI†) shows the valence band spectra of the GS and GT samples in the 0–15 eV binding energy range. The valence band maxima (VBM) results from the hybridization of the O 2p and Ga 3d orbital.53 The VBM for the GS and GT samples was estimated using the linear extrapolation method of the leading valence band edge, as shown in Fig. 2(e) and (f). The VBM was estimated to be 3.74 eV far from the Fermi level in the GS sample, as shown in Fig. 2(e), whereas, in the GT sample, it is only 2.31 eV far from the Fermi level [Fig. 2(f)]. The downward shift in the VBM of the GT sample by 1.53 eV, like that observed from the Ga 3d and O 1s core level scan, confirms the occurrence of SBB in Ga2O3 grown on p-GaN as compared to that grown on sapphire (0001).
Also, the valence band spectrum of pristine p-GaN was obtained as shown in Fig. S2(f) (see the ESI†), and the VBM was estimated to be 0.64 eV. As deduced from the PL spectra in Fig. 1(c) and (d), both PLD-grown Ga2O3 GS and GT samples have an energy band gap of ∼4.6 eV. It was surprisingly noticed from the valence band spectra that PLD-Ga2O3 grown on sapphire (0001) reveals (EVBM = 3.74 eV) unintentionally doped (UID) high n-type (n++) characteristics while that grown on p-GaN/sapphire (0001) [EVBM = 2.31 eV] reveals a very low UID n-type (n−−) character.
To understand the role of the substrate in changing the optical and electronic states of Ga2O3 theoretically, DFT calculations were performed, and the results obtained are presented in Fig. 3. The computational details of the DFT calculations are presented in the ESI.† The atom projected partial density of states (pDOS) of pristine and defective Ga2O3 with single O-vacancy and N-substitution have been plotted as shown in Fig. 3(b)–(d), respectively. In pristine Ga2O3, the O-orbitals predominantly contribute to the valence band states, whereas Ga-orbitals contribute to the conduction band states (see Fig. 3(b)). The Fermi level is near the conduction band. In reality, some defects, for instance O-vacancies and N-related defects, might be present unintentionally due to the use of different substrates (here, GaN). With the creation of a single O-vacancy in the Ga2O3 supercell, some defect states appear near the valence band, leading to a decrease in the band gap. This result corroborates our experimental findings of PL measurement, as shown in Fig. 1(c) and (d). These defect states are contributed by both O- and Ga-orbitals (see Fig. 3(c)). The decrease varies across three inequivalent O-sites (see Fig. 3(a) for inequivalent O-sites). The pDOS for the same is shown in Fig. S3(a) and (b) (ESI†). These localized states efficiently trap the minority charge carriers (holes), enhancing the photo-generated charge carriers' separation and recombination time. This leads to persistent photoconductivity in Ga2O3. However, when N is substituted at this site (which was previously O-vacant), the localized states, contributed by N-orbitals, move towards the VBM (see Fig. 3(d)) and appear at the VBM in the case of different N-sites (Fig. S3(c) and (d), ESI†). Hence, the trapped defect states are smaller in the GT sample, which is experimentally depicted in the PL spectrum (see Fig. 1(d)). Furthermore, the distance of the Fermi level from the valence band decreases, which is also observed experimentally in the valence band spectra (see Fig. 2(f)). As N has one electron less than O, it acts as an acceptor. Furthermore, from Fig. 3(d), we can see that the Fermi level (fixed at 0 eV) in N-substituted Ga2O3 has shifted inside the valence band, indicating the availability of free holes. Therefore, in the case of the GT sample, we have a lower n−− character, leading to a decrease in the persistent photoconductivity and enhancing the response of the photodetector device.
Fig. 3 (a) Crystal structure of Ga2O3. Atom projected partial density of states of (b) pristine, (c) O-vacant (O-vacancy at the O3-site), and (d) N-substituted Ga2O3 (N-substitution at the O3-site). |
Next, we fabricated MSM PDs to compare the photo response quality of the PLD-grown Ga2O3 GS and GT samples [Fig. S4, ESI†]. The photoresponse results reveal that the GT device can detect light in a broad UV region varying from the UV C to UV A region of the wavelength spectrum with a higher photoresponse than the GS device, as presented in Fig. S4(d) (ESI†).
Furthermore, to make an ultra-broadband PD, we have utilized a vdW 2D/3D heterostructure by depositing a MoSe2 thin film via magnetron sputtering on PLD-grown Ga2O3 GS and GT samples and named them MGS and MGT, respectively. Fig. 4(a) displays the Raman spectra of MGS and MGT in the 100 to 800 cm−1 range. In Fig. 4(a), the presence of distinctive A1g and E12g phonon modes at Raman shifts of 236.1 (237.2) and 289.8 (286.5) cm−1, respectively, are the signature Raman peaks of MoSe2, which confirm the formation of MoSe2 on the GS (GT) sample.54 Furthermore, the Raman peaks at locations 155.2 (154.1) and 193.0 (194.1) cm−1 are assigned to the A2(g) and A3(g) modes of β-Ga2O3 in the MGS (MGT) sample, and the Raman peaks marked with asterisks correspond to the sapphire substrate.39,41 In addition, the sharp and high-intensity Raman peaks recorded at 568.1 and 737.2 cm−1 in the MGT sample are attributed to the E2 (high) and A1 (LO) phonon modes of GaN.44 Furthermore, to determine the atomic ratio of the sputtered MoSe2 thin film, EDS elemental analysis was performed. Fig. 4(b) represents the graph of the atomic percentage of the elements present in the MoSe2 thin film. The atomic ratio of 1:1.98 of Mo and Se revealed a suitable stoichiometry after the post-selenization of the magnetron-sputtered MoSe2 thin film. Furthermore, the morphology of the MGS and MGT samples was examined by performing high-magnification FESEM image scans, as shown in Fig. 4(c) and (d). The FESEM images of MoSe2 grown on PLD-grown Ga2O3 confirm the formation of worm-like structures of magnetron-sputtered MoSe2 thin film, with uniform coverage over the entire scanned sample surfaces. The magnetron-sputtered TMD thin films were seen to have worm-like surface morphology because they first grow in a vertical direction. After reaching a specific thickness, their growth occurs in a lateral direction, forming worm-like structures.55 Furthermore, to examine the surface roughness of the magnetron sputtered MoSe2 thin film deposited on the PLD-grown β-Ga2O3 samples, we conducted AFM scans, as shown in Fig. S5(a) and (b) (ESI†).
Fig. 4 (a) Raman spectra, (b) EDS atomic percentage, (c) and (d) plane view FESEM images, (e) XPS Mo 3d core level scan, and (f) valence band spectra of the MGS and MGT samples. |
The AFM imaging also compliments the worm-type MoSe2 morphology, as shown in Fig. 4(c) and (d). The roughness of the MGS and MGT samples was estimated to be 7.37 and 5.42 nm, respectively. The low roughness value of MGT reveals a smoother surface than that of MGS. We conducted an XPS measurement of the Mo and Se core levels to study the chemical composition of the as-grown MoSe2/Ga2O3 MGS and MGT samples. The core level Mo 3d and Se 3d scans for the MGS and MGT samples are presented in Fig. 4(e). The two broad peaks in the MGS and MGT samples are noticed to be shifted by a small value of binding energy. To determine the valence state of each element, we further deconvoluted it with a Voigt function and Sherley background. Fig. S6(a) and (b) (ESI†) show deconvoluted Mo 3d core level spectra presenting different valence states of Mo element present on the surface of the MGS and MGT samples, respectively. It shows the apparent appearance of Mo and Se on the surface of the MoSe2 film and confirms the formation of the 2H-MoSe2 phase.56,57 The Voigt function fitted Se 3d spectra of the MGS and MGT samples are illustrated in Fig. S6(c) and (d) (ESI†). The peak position and FWHM of each deconvoluted peak are presented in Table S1 (ESI†). Furthermore, no peak corresponding to Mo–Ga or Se–Ga was observed in the XPS spectra of the MGS and MGT samples [Fig. S6, ESI†], which suggests that MoSe2 is not attached to Ga2O3 by any chemical bonding but rather by weak van der Waals forces. Furthermore, the valence band maxima (VBM) calculated in the MGS and MGT samples are 0.20 and 0.22 eV, respectively [Fig. 4(f)], which reveals that the Fermi levels have nearly identical energy in both the MoSe2 samples.
Furthermore, to study the photodetection properties of these heterostructures, we fabricated single and dual junction photodetector devices on MoSe2/n-Ga2O3/sapphire (MGS) and MoSe2/n-Ga2O3/p-GaN (MGT), respectively. A typical I–V curve of the hybrid MGS and MGT device was performed for −10 to 10 V, as presented in Fig. S7(a) and (b) (ESI†), respectively. To understand the photodetection properties of the fabricated devices at different wavelength regions of the electromagnetic spectrum, we have determined the time–dependent current (I–t) characteristics. The I–t characteristics were conducted at various applied biases from 0.5 to 10 V with laser light ON and OFF cycles taken to be 10 s. Fig. 5 shows the MGS device's I–t characteristics curve measurements under 255 nm and 1064 nm illumination. Fig. 5(a) displays the I–t curves at 255 nm laser illumination at various voltages of 0.5 to 10 V. The current is enhanced with a rise in externally applied voltage, as discussed in the previous section, and the cycles are repeatable and stable over multiple cycles of light ON and OFF. The photocurrent was seen to rise and become stable when the laser was illuminated quickly. After removing the laser light, the photocurrent reached its minimum value, which revealed that the device had a faster response time. The response (τr) and decay (τd) times of the device are estimated by fitting using the following equations:
(1) |
(2) |
Furthermore, the performance of a photodetector is evaluated using photodetection parameters such as responsivity and detectivity. The values of these performance parameters were estimated using the following equations:
(3) |
(4) |
Device | Under 255 nm | Under 355 nm | Under 1064 nm | ||||||
---|---|---|---|---|---|---|---|---|---|
Responsivity (A W−1)/detectivity (×109 Jones) | Response time (s) | Responsivity (A W−1)/detectivity (×109 Jones) | Response time (s) | Responsivity (A W−1)/detectivity (×109 Jones) | Response time (s) | ||||
Rise (τr) | Decay (τd) | Rise (τr) | Decay (τd) | Rise (τr) | Decay (τd) | ||||
MGS | 18.1/2.4 | 0.43 | 0.69 | — | — | — | 1.4/0.2 | 0.77 | 1.06 |
MGT | 32.7/3.2 | 0.55 | 0.76 | 25.2/2.7 | 0.68 | 0.81 | 5.5/0.5 | 1.21 | 1.24 |
Furthermore, the MGS device underwent I–t curve measurements with 1064 nm laser light illumination, as shown in Fig. 5(d). The device's maximum current was measured at a voltage of 10 V to be 16.8 μA. The rise and decay time of the MGS device under the illumination of 1064 nm laser light was estimated using eqn (1) and (2), as shown in Fig. 5(e), and the values of rise and decay times are estimated to be 0.77 s and 1.06 s, respectively. It can be seen that the MGS device shows a similar time response under different laser light illumination. Furthermore, the responsivity and detectivity of the MGS device under 1064 nm laser light were estimated at various applied biases using eqn (3) and (4) and plotted in Fig. 5(f). The estimated values of responsivity and detectivity at 10 V were 1.4 A W−1 and 1.8 × 108 Jones, respectively. The values of the figures of merit of the MGS device under 1064 nm light illumination are displayed in Table 2.
It was observed from the spectral response in Fig. S4(d) (ESI†) that the introduction of p-GaN not only enhances the response of the device in DUV regions but also broadens the range of photodetection in UV regions due to the active GaN semiconducting material, which responds in the UV A region. Hence, photo response I–t curve measurements for the MGT device were performed at different laser wavelengths, as shown in Fig. 6. Fig. 6(a) shows the I–t curve of the MGT device under multiple ON/OFF cycles of laser illumination at wavelengths of 255 nm and 355 nm at a low voltage of 0.1 V. The photocurrent measured under wavelengths of 255 and 355 nm was 0.25 and 0.15 μA, respectively. Next, Fig. 6(b) displays the I–t curve of the MGT device under wavelengths of 255 nm and 355 nm at voltages varying from 0.5 to 10 V. The maximum photocurrent measured at 10 V of externally applied voltage is 25 μA. The value of photocurrent corresponding to the MGT device was nearly double that of the MGS device at the same parameters under 255 nm laser illumination. This enhancement in responsivity of the MGT device as compared to MGS is due to the presence of p-GaN over the sapphire (0001), which boosts the photocurrent by nearly 100% because here both Ga2O3 and GaN are active materials in response to 255 nm laser light. Additionally, the photocurrent of the MGT device under 355 nm wavelength illumination was 17 μA at 10 V, which is lower than that measured under a 255 nm laser because only GaN is an active material for 355 nm laser light, unlike at 255 nm. Furthermore, the time response was calculated using eqn (1) and (2) for the MGT device under 255 and 355 nm light illumination and displayed in Fig. 6(c) and (d), respectively. The estimated values of rise and decay time are 0.55 (0.68) s and 0.76 (0.81) s, respectively, under 255 (355) nm laser illumination. The responsivity and detectivity of the MGT device were calculated at various applied voltages under 255 nm laser light illumination and plotted as shown in Fig. 6(e). The responsivity and detectivity estimated values at 10 V are 32.7 A W−1 and 3.2 × 109 Jones, respectively. Furthermore, the responsivity and detectivity calculated under 355 nm light illumination at various applied biases are shown in Fig. 6(f). The responsivity and detectivity measured at 10 V are 25.2 A W−1 and 2.7 × 109 Jones, respectively. The values of various figures of merit of the MGT device are presented in Table 2. In our work, we have found that the responsivity of PD devices is higher compared to the ones that have been recently fabricated using UWBG semiconductors.17,39,58–64 A comparison table of our work with other studies is presented in Table 3.
Heterojunction | Growth technique | Responsivity | Ref. |
---|---|---|---|
n-Ga2O3/SiC | MBE | 18 mA W−1@−10 V | 17 |
n-Ga2O3/p-GaN | Gallium evaporation in oxygen plasma | 0.18 A W−1 | 39 |
AlGaN | MOCVD | 0.19 A W−1@−5 V | 59 |
n-Ga2O3/ZnO | Magnetron sputtering | 0.35 A W−1@5 V | 60 |
n-Ga2O3/GaN | CVD | 27.5 mA W−1@10 V | 61 |
Amorphous Ga2O3/PET | Magnetron sputtering | 8.9 A W−1@15 V | 62 |
MgZnO | MOCVD | 100 mA W−1@30 V | 63 |
p-Ga2O3/n-GaN | Thermal oxidation | 56 A W−1@−5 V | 64 |
n-Ga2O3/p-GaN | PLD | 32.7 A W−1 at 10 V | This work |
Furthermore, the MGT device was characterized using 1064 nm laser light. Fig. 7(a) shows the I–t curve at a low voltage of 0.1 V. Fig. 7(b) shows the I–t curves at various applied biases ranging from 0.5 to 10 V. The maximum photocurrent was observed to be 65 μA at 10 V, which is four times higher than that observed for MGS under the same parameters and illumination of the same laser. This 4-fold enhancement in photocurrent of the MGT device reveals the significance of the presence of p-GaN. Fig. 7(c) shows the fitted time response of the MGT device under 1064 wavelength laser illumination, and the fitted value of the rise and decay times was calculated to be 1.21 and 1.24 s, respectively. Furthermore, the voltage-dependent graph of estimated responsivity and detectivity of the MGT device under 1064 nm is shown in Fig. 7(d), and the maximum responsivity found at 10 V is 5.5 A W−1 and 5.4 × 108 Jones, respectively. It was observed that the photoresponsivity of the MGT device is higher than that of the MGS device at each region of the electromagnetic spectrum.
The mechanism of enhancement in the photoresponse characteristics of the MGT device compared to the MGS device is shown in Fig. 8. Fig. 8(a) and (b) represent the cross-sectional view of the GS and GT samples, respectively. It was revealed from the valence band spectra of the GS and GT samples that they have UID n++ and n−− characteristics, respectively, which were theoretically confirmed by DFT calculation. Therefore, a p–n−− type heterojunction is formed in the MGT device between Ga2O3 (n−−) and GaN (p). Further, it is well known that if we join a low-doped semiconductor with a high-doped material, the depletion region or space charge region will be more on the low-doped semiconductor side. In the GS sample, Ga2O3 is not attached to any doped semiconductor; in the GT sample, it is grown on a p-type doped GaN semiconductor. Hence, the built-in electric field developed at the interface of the Ga2O3/GaN p–n−− junction will be spread over a large region on the Ga2O3 side (marked with a broken line region in black color) as shown in Fig. 8(b), while it is absent in the Ga2O3 GS sample.
Fig. 8 Schematic diagram of the space charge region formed at the interface of the (a) GS and (b) GT samples. Charge transport mechanism under the illumination of (c) MGS and (d) MGT devices. |
Furthermore, Fig. 8(c) and (d) show the side views of the MGS and MGT devices, respectively. Fig. 8(c) shows that a built-in electric field is present at the interface of MoSe2 and n-Ga2O3 due to the charge transfer in each other. Therefore, electron–hole pairs are generated in both semiconductors when the light is incident on the MGS device with hν > Eg (Ga2O3). In an externally applied field, electrons drift toward the electrode from both the semiconductors.
However, it was observed that the built-in-electric field is present at the interface under the influence of which some of the charge carriers from Ga2O3 drift towards electrodes through MoSe2. However, the electrons buried under some thickness near the bottom of the Ga2O3 semiconductor cannot reach the electrode. Instead, they recombine with the hole and annihilate as the built-in electric field is insufficient to drift them toward electrodes, as represented by a circle in Fig. 8(c), which limits the photoresponse properties of the GS sample.
Moreover, in Fig. 8(d), in addition to the built-in electric field developed at the interface due to the vdW heterostructure between MoSe2 and n-Ga2O3, there is an extra built-in electric field present at the interface of the UID n−− Ga2O3 and p-doped GaN template. This extra electric field in the MGT device pushes these buried electrons in Ga2O3 to reach their respective electrodes without undergoing recombination with the photogenerated holes, and the diminished recombination of photogenerated charge carriers leads to improvement in photocurrent in the external circuit. Furthermore, the MGT device demonstrated higher photoresponse properties and exhibited a higher responsivity in the UV A region under 355 nm light illumination compared with MGS. Furthermore, the MGT device shows over four times higher photocurrent than MGS when illuminated with 1064 nm light. This is evidence that the built-in electric field at the interface of n-Ga2O3 and p-GaN plays a supportive role in efficiently separating the photogenerated charge carriers, significantly improving the photo response properties of the MGT device. Furthermore, the better crystalline, optical, and structural qualities of Ga2O3/p-GaN lead to the higher photoresponse properties of the MGT device compared to MGS. In conclusion, dual junction photodetectors are more efficient and work in a wide range of electromagnetic spectra, which makes them useful for futuristic optoelectronic applications.
Footnote |
† Electronic supplementary information (ESI) available: RHEED, AFM images of Ga2O3 [Fig. S1], PL and XPS of Ga2O3 and p-GaN templates [Fig. S2], DFT partial density of states in Ga2O3 [Fig. S3], photodetector characteristics of bare Ga2O3 [Fig. S4], AFM, XPS, and I–V characteristics of MoSe2/Ga2O3 [Fig. S5–S7]. Table S1 contains the peak positions of XPS spectrum MoSe2/Ga2O3 samples. See DOI: https://doi.org/10.1039/d4ma00934g |
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