Metal-first non-alloyed ohmic and Schottky contacts are fabricated on β-Ga 2O 3 with a range of metal work functions ( ϕ M). The resulting ohmic contacts are of high quality with a contact resistance ( R c) as low as 0.069 ± 0.003 Ω mm. Measurements of the barrier heights ( ϕ B) indicate that metal-first processing, which preserves the as-grown/bare-substrate surface, also partially un-pins the Fermi-level in (010) and ( 2 ¯01) oriented Ga 2 O 3. Depth-resolved XPS (x-ray photoelectron spectroscopy) measurements of the oxidation state throughout the contact metal at the contact– Ga 2 O 3 interface indicate that most non-alloyed contact metals are at least partially oxidized by room temperature redox reactions with the underlying Ga 2 O 3, with metals with a lower ϕ M also demonstrating the greatest level of oxidation. As oxidation has been previously observed to enhance a metal’s work function, this may imply that to-date observations of indices of surface behavior << 1 on β-Ga 2O 3, which have been attributed to severe Fermi-level pinning, may need to be corrected to account for this partial oxidation in addition to other surface modifications during device processing demonstrated in this work.

Beta-phase gallium-oxide ( β-Ga 2O 3) has been investigated in recent years as a promising material in power electronics thanks to its large estimated critical breakdown field (8 MV/cm), adequate electron mobility (200  cm 2/V s), and availability of large area substrates from melt.1–3 Impressive devices demonstrations have been recorded with a record average breakdown electric field observed in both Schottky barrier diodes (SBDs) and field-effect transistors (FETs) at 5.7 MV/cm, with surface fields as high as 6 MV/cm enabled by oxidized metal Schottky contacts with barrier heights ( ϕ B) > 2 eV.4–7 

Despite these advances, reported Schottky-barrier heights to Ga 2 O 3 through the years have demonstrated a stark lack of consistency.8 The Schottky-barrier height at a metal–semiconductor interface is nominally defined by the Schottky–Mott rule, where the barrier height is determined only by the electron affinity of the semiconductor ( χ S) and the work function of the metal ( ϕ M) according to Eq. (1),
(1)
However, experimental results have deviated from this expectation. For example, a Pt ( ϕ M 5.65 eV) to Ga 2 O 3 ( χ S 3.9 eV) contact is predicted to have a ϕ B of 1.6–1.75 eV. Nevertheless, reported values range between 0.6 and 2.2 eV.9,10 The deviation of ϕ B from the Schottky–Mott rule has been attributed to Fermi-level pinning. Furthermore, while some studies suggest that the Fermi level is fully pinned in Ga 2 O 3, others have demonstrated that ϕ B is only weakly pinned as predicted by Kurtin et al. given the ionicity of Ga 2 O 3, which is not high enough to yield the complete pinning observed in GaAs.11 This partial surface pinning has been observed in other semiconducting materials, and thus, an index of surface behavior ( S) was introduced to describe Fermi-level pinning, which modifies the Schottky–Mott rule to12 
(2)
where S = 1 corresponds to ideal Schottky–Mott behavior and S = 0 corresponds to a fully pinned surface. Fermi-level pinning in β- Ga 2 O 3 has been attributed to a number of origins, including the surface orientation, native oxygen and gallium vacancies or interstitials induced during growth, and surface defects generated during device fabrication processes, such as high temperature annealing and energetic plasma exposure.8 

Our previous work has demonstrated that conventional lift-off processing of metal contacts significantly modifies the surface of β- Ga 2 O 3 and impedes consistent and reliable ohmic contact formation, while a metal-first contact process improves both contact quality and consistency.13 Contact-first processes have also been demonstrated in prior studies, albeit not explicitly for the purpose of minimal surface modification, in ITO/AZO ohmic contacts that out-performed conventional lifted-off Ti/Au contacts reported by Carey et al., and in the ozone-MBE deposited oxidized Schottky contacts that attained 6 MV/cm reported by Cromer et al.7,14,15 Given nearly all metal contacts to Ga 2 O 3 in the literature to date were formed by lift-off, it is reasonable to assume the same or similar processing inconsistencies observed in Ti/Au ohmic contacts (Ref. 13) may have led to the wildly varied values of ϕ B and S in the literature.

In this work, we demonstrate non-alloyed, metal-first ohmic and Schottky contacts fabricated with contact metals having a range of work functions to further explore the limitations of Fermi-level pinning in β- Ga 2 O 3.We fabricated transfer length method (TLM) patterns for all six contact metals (Al, Ti, Cr, Ni, Pd, and Pt) and vertical SBDs for the high work-function metals (Ni, Pd, and Pt) and, by fitting the ohmic and Schottky IV behavior of these contacts to established emission mechanisms, are able to extract apparent specific contact resistances for metal contacts that exhibit ohmic IV characteristics and Schottky-barrier heights for both ohmic and Schottky characteristics.

The TLM patterns for all six contact metals were fabricated on two heavily n+ doped samples grown by metal–organic chemical vapor deposition (MOCVD), each diced into three pieces after growth to reduce inter-sample growth non-uniformity (samples A–F). The in situ doped samples were grown in an Agnitron Agilis 100 MOCVD system on Fe-doped (010) β-Ga 2O 3 substrates. Prior to growth, samples were ex situ etched with 48% HF for 30 min and immediately loaded.16 A 50 nm unintentionally doped buffer layer was grown first before growing the 220–250 nm highly doped layer. The samples were then diced and solvent cleaned. Further details of the MOCVD growth can be found in the supplementary material. Hall measurements on previously grown calibration samples gave a channel charge and mobility of 9 × 10 19 cm 3 and 84  cm 2/V s for samples A, D, and F and 7 × 10 19 cm 3 and 89  cm 2/V s for samples B–C and E. The metal stacks were then deposited by electron-beam evaporation. Circular TLM (CTLM) patterns were defined using contact lithography, and the metal stacks were then wet etched (see Table I for metal layer thicknesses and wet etch conditions). The detailed fabrication of metal-first ohmic contacts can be found in our prior report.13 

TABLE I.

Summary of metal/Ga2O3 samples in this study: metal stacks, nominal work function of the contact metal, and metal etch conditions.

SampleorientationNd (cm−3)Metal Stack (nm)ϕM (eV)Etchant 1Etch 1 Time (s)Etchant 2Etch 2 Time (s)
Ohmic series 
(010) 9 × 1019 Al (110) 4.2 Al etchant, type A 210 … … 
(010) 7 × 1019 Ti/Au (10/110) 4.33 Gold etchant TFA 40 30:1 BOE 90 
B′ (010) 9 × 1019 Ti/Au (10/110) 4.33 Gold etchant TFA 40 30:1 BOE 90 
(010) 7 × 1019 Cr/Au (10/110) 4.5 Gold etchant TFA 40 Cr Etch 1020 20 
(010) 9 × 1019 Ni/Au (10/110) 5.2 Gold etchant TFA 40 1:1 DI:HCl, 35 °C 60 
(010) 7 × 1019 Pd/Au (10/110) 5.4 Gold etchant TFA 40 … … 
(010) 9 × 1019 Pt/Au (10/110) 5.65 Gold etchant TFA 40 200 V ion mill 120 
SBD series 
( 2 ¯01) ∼6 × 1018 Ni/Au (10/110) 5.2 Gold etchant TFA 40 1:1 DI:HCl, 35 °C 60 
( 2 ¯01) ∼6 × 1018 Pd/Au (10/110) 5.4 Gold etchant TFA 40 … … 
( 2 ¯01) ∼6 × 1018 Pt/Au (10/110) 5.65 Gold etchant TFA 40 200 V ion mill 120 
SampleorientationNd (cm−3)Metal Stack (nm)ϕM (eV)Etchant 1Etch 1 Time (s)Etchant 2Etch 2 Time (s)
Ohmic series 
(010) 9 × 1019 Al (110) 4.2 Al etchant, type A 210 … … 
(010) 7 × 1019 Ti/Au (10/110) 4.33 Gold etchant TFA 40 30:1 BOE 90 
B′ (010) 9 × 1019 Ti/Au (10/110) 4.33 Gold etchant TFA 40 30:1 BOE 90 
(010) 7 × 1019 Cr/Au (10/110) 4.5 Gold etchant TFA 40 Cr Etch 1020 20 
(010) 9 × 1019 Ni/Au (10/110) 5.2 Gold etchant TFA 40 1:1 DI:HCl, 35 °C 60 
(010) 7 × 1019 Pd/Au (10/110) 5.4 Gold etchant TFA 40 … … 
(010) 9 × 1019 Pt/Au (10/110) 5.65 Gold etchant TFA 40 200 V ion mill 120 
SBD series 
( 2 ¯01) ∼6 × 1018 Ni/Au (10/110) 5.2 Gold etchant TFA 40 1:1 DI:HCl, 35 °C 60 
( 2 ¯01) ∼6 × 1018 Pd/Au (10/110) 5.4 Gold etchant TFA 40 … … 
( 2 ¯01) ∼6 × 1018 Pt/Au (10/110) 5.65 Gold etchant TFA 40 200 V ion mill 120 

The SBDs for the high work-function metals were fabricated on diced 1 × 1 cm 2 pieces (samples G–I) from a 2 in. ( 2 ¯01) Sn-doped β- Ga 2 O 3 substrate from Novel Crystal Technology, Inc. The fabrication process is diagrammed in Fig. S1 of the supplementary material, including a blanket backside ohmic contact, frontside blanket deposition of the Ni, Pd, or Pt followed by photolithographic and wet etch anode patterning, and a BCl 3 / Cl 2-based self-aligned mesa etch for isolation. During backside cathode deposition, the front side of the sample was protected by a blanket layer of photoresist. The protective layer was removed before cathode annealing by a long soak (>30 min) in heated ( 65  °C) 1165 Microposit Remover™. Coating and removal of a blanket photoresist layer by solvent strip has been demonstrated to still form uniform, low resistance metal-first Ti/Au ohmic contacts on n+ β- Ga 2 O 3, sample B . The process information for sample B is included in Table I, with full process information detailed in the supplementary material. An additional solvent clean in acetone and isopropanol was performed prior to frontside anode deposition. Full process details are included in the supplementary material.

The CTLM patterns were measured using a Keithley 4200 Semiconductor Characterization System in a four-point probe configuration, with an inner radius of 50  μm and TLM pad spacings from 3 to 12  μm confirmed by scanning electron microscopy. Forward I–V, reverse I–V, and C–V were measured on the SBDs using the same system in a vertical two-point configuration on devices with an anode radius of 100  μm. A Thermo-Nexsa G2 x-ray photoelectron spectrometer (XPS) with Al-K α x-ray source with in situ ion mill and electron flood gun for charge compensation was used to measure the oxidation state of the metal contact at the metal–semiconductor interface.

Figure 1(a) shows the I–V curves from an example CTLM pattern with 5  μm spacing for samples A–F. The low work-function contacts (samples A–C) are linear or nearly linear ohmic with the resistance apparently increasing with increasing ϕ M of the contact metal from Al ( ϕ M = 4.2 eV) to Cr ( ϕ M = 4.5 eV). The high work-function metals (samples D–F) show varying degrees of Schottky behavior. From sampling at least four sets of TLM patterns per sample, we find that the Al contacts have an average non-alloyed R c of 0.069 ± 0.003 Ω mm, which leads to a specific contact resistance ( ρ c) of 1.1 ± 0.1 × 10 6 Ω-cm 2 [Figs. 1(b)1(c)]. Notably, R c is constant over the entire 100 mA measurement range [Fig. 1(b)]. This is among the lowest reported contact resistances on (010) β-Ga 2O 3. These Al-based contacts, as well as the Ti and Cr contacts, are benchmarked in Fig. 2. Further improvements in contact resistance can be anticipated by increasing to doping densities beyond 1 × 10 20 cm 3 and by refining surface cleanliness. Thermal stability of these metal-first interfaces also remains an open question beyond the scope of this work.

FIG. 1.

(a) I–V curves for an example CTLM pattern with a 5  μm spacing for Al (red), Ti (orange), Cr (yellow), Ni (green), Pd (blue), and Pt (purple) contacts. Al and Ti have linear ohmic behavior, while Cr has nearly-linear ohmic behavior. Ni, Pd, and Pt all have Schottky I–V behavior. (b) Extraction of R c and R s h for Al contacts from 0 to 100 mA applied current bias. R c is effectively constant at 0.069 ± 0.003 Ω mm ( 1.1 ± 0.1 × 10 6 Ω cm 2) after averaging over four sets of CTLM patterns. (c) Extraction of ρ c at 0 mA applied bias for Al, Ti, and Cr contacts on an example CTLM set gives 0.063  Ω mm ( 8.0 × 10 7 Ω cm 2), 0.46  Ω mm 2.8 × 10 5 ( Ω cm 2), and 0.77  Ω mm ( 9.6 × 10 5 Ω cm 2), respectively.

FIG. 1.

(a) I–V curves for an example CTLM pattern with a 5  μm spacing for Al (red), Ti (orange), Cr (yellow), Ni (green), Pd (blue), and Pt (purple) contacts. Al and Ti have linear ohmic behavior, while Cr has nearly-linear ohmic behavior. Ni, Pd, and Pt all have Schottky I–V behavior. (b) Extraction of R c and R s h for Al contacts from 0 to 100 mA applied current bias. R c is effectively constant at 0.069 ± 0.003 Ω mm ( 1.1 ± 0.1 × 10 6 Ω cm 2) after averaging over four sets of CTLM patterns. (c) Extraction of ρ c at 0 mA applied bias for Al, Ti, and Cr contacts on an example CTLM set gives 0.063  Ω mm ( 8.0 × 10 7 Ω cm 2), 0.46  Ω mm 2.8 × 10 5 ( Ω cm 2), and 0.77  Ω mm ( 9.6 × 10 5 Ω cm 2), respectively.

Close modal
FIG. 2.

Benchmarking of Al, Ti, and Cr ohmic contacts to (010) β-Ga 2O 3. The historical data used in this plot are tabulated in the supplementary material.

FIG. 2.

Benchmarking of Al, Ti, and Cr ohmic contacts to (010) β-Ga 2O 3. The historical data used in this plot are tabulated in the supplementary material.

Close modal

The Ti and Cr contacts on samples B and C have a higher average non-alloyed R c of 0.48 ± 0.01  Ω-mm and 0.80 ± 0.01  Ω-mm, respectively, with a corresponding ρ c of 2.9 ± 0.1 × 10 5 Ω cm 2 and 1.1 ± 0.1 × 10 4 Ω cm 2. These results are summarized in Table II. The Ti/Au contacts on sample B are also linear and ohmic, with a non-alloyed R c and corresponding ρ c of 0.18 ± 0.01  Ω-mm and 6.5 ± 0.6 × 10 6 Ω- cm 2, respectively. These contacts are also included in Table II and Fig. 2, with a full discussion of the contact behavior included in the supplementary material. The Ni, Pd, and Pt contacts do not show linear I–V behavior, and thus, a contact resistance is not extracted.

TABLE II.

Summary of extracted barrier heights for metal/Ga2O3 interfaces in this work.

Ohmic series
SampleContact metalϕM (eV)ϕB,FIV (eV)Rc (Ω mm)ρc (Ω cm2)
Al 4.2 0.27 ± 0.03 0.069 ± 0.003 1.1 ± 0.1×10−6 
Ti 4.33 0.57 ± 0.01 0.48 ± 0.01 2.9 ± 0.1×10−5 
B′ Ti 4.33 0.59 ± 0.01 0.18 ± 0.01 6.5 ± 0.6×10−6 
Cr 4.5 0.69 ± 0.01 0.80 ± 0.01 1.1 ± 0.1×10−4 
SBD series 
    ϕB,RIV ϕB,CV 
    (eV) (eV) 
Ni 5.2 1.08 ± 0.12 1.10 ± 0.11 1.31 ± 0.01 
Pd 5.4 1.46 ± 0.02 1.44 ± 0.01 1.71 ± 0.25 
Pt 5.65 1.32 ± 0.02 1.33 ± 0.02 1.43 ± 0.11 
Ohmic series
SampleContact metalϕM (eV)ϕB,FIV (eV)Rc (Ω mm)ρc (Ω cm2)
Al 4.2 0.27 ± 0.03 0.069 ± 0.003 1.1 ± 0.1×10−6 
Ti 4.33 0.57 ± 0.01 0.48 ± 0.01 2.9 ± 0.1×10−5 
B′ Ti 4.33 0.59 ± 0.01 0.18 ± 0.01 6.5 ± 0.6×10−6 
Cr 4.5 0.69 ± 0.01 0.80 ± 0.01 1.1 ± 0.1×10−4 
SBD series 
    ϕB,RIV ϕB,CV 
    (eV) (eV) 
Ni 5.2 1.08 ± 0.12 1.10 ± 0.11 1.31 ± 0.01 
Pd 5.4 1.46 ± 0.02 1.44 ± 0.01 1.71 ± 0.25 
Pt 5.65 1.32 ± 0.02 1.33 ± 0.02 1.43 ± 0.11 
At zero bias, the specific contact resistance is determined from the J–V behavior of the contact according to18 
(3)
In order to apply this relation to our ohmic contacts, we must first determine which mechanism dominates forward conduction at low applied bias. As all the metal contacts fabricated here, regardless of I–V behavior, ought to exhibit a Schottky barrier, we have three mechanisms to consider: thermionic emission (TE) over the barrier, field emission (FE) tunneling through the barrier, or thermionic-field emission (TFE), which combines the two. We can then identify the appropriate expression for J. The criteria used to distinguish between conduction regimes is typically related to the surface electric field (F s u r f). As ρ c is reported here at 0 bias, we will reference our criteria to the surface electric field at 0 bias, F 0, which is given by19 
(4)
with ϵ s, k B, T, and N d assuming their typical meanings and V bi being the built-in voltage. Often, a simplified version of V bi, V bi, 0 = ϕ B is used. However, for degenerately doped semiconductors, additional considerations must be made.
In degenerate semiconductors, E \,f lies above E c. The normally unoccupied states above the conduction band minimum but below E \,f are occupied by electrons, i.e., the Burstein–Moss (BM) band filling effect ( Δ E BM), leading to an expansion in the optical absorption bandgap ( E g, opt). In addition, bandgap renormalization ( Δ E BGR = Δ E BGR, C + Δ E BGR, V) occurs due to electron–electron ( Δ E ee) and electron–dopant ( Δ E ei) Coulomb interactions, which narrow the bandgap.17,20 Both BM band filling and bandgap renormalization (BGR) depend on doping concentration. Figure 3(a) sketches the impacts of both of these effects on the semiconductor band structure. The expressions for Δ E BM and Δ E BGR are described in the supplementary material and plotted in Fig. S2 of the supplementary material. However, the net optical absorption bandgap plotted in Fig. S2 of the supplementary material is not the critical parameter in this study, but instead (1) V bi, which is determined by the relative difference between ϕ M and E \,f in the bulk Ga 2 O 3, and (2) ϕ B, which is controlled by the location of the conduction band edge E c relative to ϕ M at the contact interface. To address the first question, from the band diagram of the bulk in Fig. 3(b), we can quickly observe that
(5)
with V bi, 0 being the built-in potential of the metal–semiconductor junction if E \,f of the semiconductor bulk is at E c, 0—a common assumption made for a degenerate semiconductor. The quantities Δ E BM and Δ E BGR are described in the supplementary material.
FIG. 3.

Illustrative diagrams (not to scale) (a) with and without the Burstein–Moss effect and bandgap renormalization applied. The BM shift occurs entirely in the conduction band, while band renormalization ( Δ E BGR = Δ E BGR, C + Δ E BGR, V) is divided between the conduction and valence bands (not necessarily evenly). The new optical absorption bandgap is measured from the valence band maximum to the Fermi level due to Burstein–Moss. (b) Band diagram showing the band structure in the metal contact, the depletion region, and semiconductor bulk taking into account BM and BGR in degenerate semiconductors. BGR is only applied in the bulk due to a lack of electron–electron interactions in the depletion region and is sketched only in the conduction band due to the observations made by Zhang et al. from DFT.17 The new V bi is also highlighted.

FIG. 3.

Illustrative diagrams (not to scale) (a) with and without the Burstein–Moss effect and bandgap renormalization applied. The BM shift occurs entirely in the conduction band, while band renormalization ( Δ E BGR = Δ E BGR, C + Δ E BGR, V) is divided between the conduction and valence bands (not necessarily evenly). The new optical absorption bandgap is measured from the valence band maximum to the Fermi level due to Burstein–Moss. (b) Band diagram showing the band structure in the metal contact, the depletion region, and semiconductor bulk taking into account BM and BGR in degenerate semiconductors. BGR is only applied in the bulk due to a lack of electron–electron interactions in the depletion region and is sketched only in the conduction band due to the observations made by Zhang et al. from DFT.17 The new V bi is also highlighted.

Close modal

As for the second point, Zhang et al. further carried out hybrid DFT calculations and determined that the conduction band edge is minimally impacted by bandgap renormalization resulting from electron-impurity interactions ( Δ E ei) due to minimal hybridization between the Si 3s and Ga 4s state that forms the basis of the conduction band minimum.17 Therefore, all bandgap renormalization ( Δ E BGR) may be attributed to electron–electron interactions ( Δ E ee). As electron–electron interactions are largely absent in the depletion region near the metal–semiconductor contact interface, we anticipate no bandgap renormalization at the interface, and therefore, the location of E c relative to ϕ M (and, therefore, ϕ B) is unaffected. In the bulk, bandgap renormalization is predominantly seen through lowering of the conduction band minimum due to the dispersive Ga 4s state from which the conduction band is derived compared to the flat valence band edge. Thus, Δ E BGR = Δ E BGR, C for n+ Ga 2O 3 doped with Si and is sketched entirely in the conduction band in Fig. 3(b).17 

With V bi and F 0 established, we can now apply the electric field criteria to determine which conduction regime applies to our contacts: TE, TFE, or FE. In the FE dominated current region, Padovani and Stratton’s criteria requires that21 
(6)
As we determine contact resistance near zero bias, F F 0 and TFE will dominate over FE as long as q ϕ B > several k B T. With such low barrier heights predicted by Schottky–Mott, it is then important to distinguish whether TFE or TE current dominates. To determine the appropriate conduction regime, we use the transition electric field F T described by Li et al. for Ga 2 O 3 below which TE dominates,19 
(7)
At the doping concentrations used for this study ( > 5 × 10 19 cm 3), F 0 > F T holds even for barriers as small as 1.15 × k B T or 30 meV at room temperature. Even at 600 K, the cutoff for ϕ B to transition from the TE to TFE regime is 1.4 × k B T or 36 meV at room temperature. These criteria are shown in Fig. S2 of the supplementary material. Based on these criteria, the dominant mode of conduction in the ohmic contacts in this study is TFE. The TFE model for the current density under forward bias V F is laid out in Eqs. (8)–(10), with A being Richardson’s constant for Ga 2 O 3,21,22
(8)
(9)
(10)
In Eq. (9), we use the modified expression for m described in the supplementary material due to mild nonparabolicity in the conduction band. In the original TFE formulation by Padovani and Stratton, the BM band filling energy ξ 2 is considered, while the effect of BGR is neglected; thus, V bi = V bi, 0 + ξ 2. However, in this study, it is necessary to consider the BGR effect as it is sizable in comparison with the barrier height (<1 eV) we expect from the ohmic contact characteristics. We correct the expression for V bi according to Eq. (5) to account for this effect, from which we see that
(11)
By applying Eq. (3), J TFE can be used to attain an expression for ρ c, TFE, substituting for ξ 2 according to Eq. (11),18 
(12)

Using the extracted specific contact resistance from TLM, ϕ B can be solved for numerically. We attain barrier heights for Al, Ti, and Cr of 0.29 ± 0.03, 0.57 ± 0.01, and 0.69 ± 0.01 eV, respectively. These, and all extracted barrier heights, are listed in Table II. The values of ϕ B monotonically increase with increasing ϕ M. Similar analysis applied to Ti contacts on 3 × 10 19, 7 × 10 19, and 8 × 10 19 cm 3 Si-doped β-Ga 2O 3 reported in our previous work yields similar barrier heights of 0.60, 0.54, and 0.56 eV, respectively, to the extracted ϕ B for Ti of 0.57 eV reported here.13 

Neglecting both BM and BGR (i.e., setting E \,f at E c in the bulk ignoring renormalization effects, as is commonly assumed for degenerate semiconductors), the extracted ϕ B is 40 meV higher than the values extracted here as, at doping densities 5 - 10 × 10 19 cm 3, the competing effects of BM and BGR on V bi are approximately equal in magnitude and, therefore, nearly cancel out. Including BM but neglecting BGR, which is most commonly seen in the literature when applying the equation by Padovani and Stratton, leads to significantly larger barrier heights by 0.5–0.6 eV due to the artificial increase in V bi.

For the rectifying Ni, Pt, and Pd contacts, we fabricated SBDs to extract barrier height and used three different methods to extract the barrier height: C–V, forward J–V fitted with the TFE model, and reverse J–V fitted with a numerical tunneling model developed by Li et al.19,23 The room temperature C–V measurements are fit according to Eq. (13) with ϵ s = 10 ϵ 0 for β-Ga 2O 3 and N d and ϕ B, CV as fitting parameters,
(13)

The extracted N d and ϕ B, CV were 5.58 × 10 18 cm 3 and 1.31 ± 0.01 eV for Ni, 6.93 × 10 18 cm 3 and 1.71 ± 0.25 eV for Pd, and 6.52 × 10 18 cm 3 and 1.43 ± 0.11 eV for Pt.

The forward J–V characteristics of the diodes in the exponential region are fit with the TFE model according to Eqs. (8)–(10), with N d set to the value extracted by C–V, V F as the independent variable, and ϕ B, FIV as the only fitting parameter. The agreement of forward J–V characteristics and the TFE model is shown in Fig. 4(b). The extracted values of ϕ B, FIV for Ni, Pd, and Pt are 1.08 ± 0.12, 1.46 ± 0.02, and 1.32 ± 0.02 eV, respectively. Unlike for the heavily degenerately doped ohmic contacts, neglecting BM and/or BGR results in a minimal shift ( 20 meV) in the extracted ϕ B as the doping density in these samples is similar to the conduction band density of states in β-Ga 2O 3, meaning that the samples are barely degenerately doped and E \,f = E c is a reasonable approximation.

FIG. 4.

(a) Reverse J–V characteristics of example Ni (green), Pd (blue), and Pt (purple) SBDs with numerical reverse leakage model fits overlaid (solid). (b) Forward J–V characteristics of example Ni, Pd, and Pt SBDs with TFE model fits overlaid.

FIG. 4.

(a) Reverse J–V characteristics of example Ni (green), Pd (blue), and Pt (purple) SBDs with numerical reverse leakage model fits overlaid (solid). (b) Forward J–V characteristics of example Ni, Pd, and Pt SBDs with TFE model fits overlaid.

Close modal

The reverse J–V characteristics of the SBDs are fit using the numerical reverse leakage model developed by Li et al. (described in the supplementary material), which incorporates doping effects and image force lowering (IFL) into the models developed by Murphy and Good and expanded by Padovani and Stratton.19,21,24 For fitting to the measured reverse J–V characteristics, V R is related to F surf according to F surf = 2 q N d ( ϕ B, RIV V R ) / ϵ s, with N d again set to the value extracted from C–V. This leaves V R as the independent variable and ϕ B, RIV as the only fitting parameter. The agreement of reverse J–V characteristics and the numerical tunneling model is shown in Fig. 4(a). The extracted values of ϕ B, RIV for Ni, Pd, and Pt are 1.10 ± 0.11, 1.44 ± 0.01, and 1.33 ± 0.02 eV, respectively.

Figure 5 plots the extracted barrier heights for Al, Ti, Cr, Ni, Pd, and Pt on Ga 2 O 3 vs their respective metal work function with prior published data. Prior studies imply that the measured barrier height on Ga 2 O 3 is heavily pinned and collectively demonstrate a minimal dependence on the work function of the contact metal. In this work, overall, we observe ϕ Al < ϕ Ti < ϕ Cr < ϕ Ni < ϕ {Pt} < ϕ Pd, which trends with increasing ϕ M with the exception of Pd and Pt (5.4 vs 5.65 eV), which are reversed. Fitting these extracted barriers to the modified Schottky–Mott rule in Eq. (2) gives S = 0.7 ± 0.2 with an R 2 of 0.85. For the barriers extracted by multiple methods, as is often observed, the barrier heights extracted by C–V are slightly higher than the barriers extracted from forward and reverse J–V.25 The barrier heights, however, obey the same trend for all barrier height extraction methods.

FIG. 5.

Measured ϕ B vs ϕ M from the literature (gray) and this work (red). Only the orientations used in this work, (010) and ( 2 ¯01) are included, with the data sorted by surface orientation and the type of measurement. This work shows ϕ B largely increases with increasing ϕ M, while measurements from the literature show significant Fermi-level pinning. Values from the literature and associated references are tabulated in the supplementary material. The overall S value based on this work alone (the red symbols) is 0.66 ± 0.03, and R 2 of 0.77 though the fitted line is not shown in this plot.

FIG. 5.

Measured ϕ B vs ϕ M from the literature (gray) and this work (red). Only the orientations used in this work, (010) and ( 2 ¯01) are included, with the data sorted by surface orientation and the type of measurement. This work shows ϕ B largely increases with increasing ϕ M, while measurements from the literature show significant Fermi-level pinning. Values from the literature and associated references are tabulated in the supplementary material. The overall S value based on this work alone (the red symbols) is 0.66 ± 0.03, and R 2 of 0.77 though the fitted line is not shown in this plot.

Close modal

Surface orientation and interface chemistry may both play a role in the observation of S-values less than 1. Previous work has indicated that Fermi-level pinning and Schottky barrier height can depend on the surface crystal orientation due to the low level of crystal symmetry in Ga 2 O 3, which results in different surface energies and density of surface states.26 On the (100) surface of Ga 2 O 3, for example, Lyle et al. demonstrated a significantly lower amount of Fermi-level pinning with S values ranging from 0.7 to 0.97, while Lingaparthi et al. obtained a similar value of S 0.66 on the (001) surface.27,28 In contrast, Hou et al. observe near complete Fermi-level pinning ( S 0) on the ( 2 ¯01) and (010) surface, which was attributed to the large number of oxygen dangling bonds on this face.6 On the (010) surface, Farzana et al. do observe a spread of Schottky-barrier heights, though they do not trend as predicted by the Schottky–Mott rule (albeit within a fairly small data set), indicating that Fermi-level pinning may not dominate Schottky-barrier formation.29 Our observation of a positive S value of 0.7 indicates that apparent Fermi-level pinning can at least be somewhat alleviated by processing techniques that preserve as-grown interface quality even on these historically pinned surface orientations. However, as this work does span two different crystal orientations, (010) and ( 2 ¯01), further work should investigate more closely Fermi-level pinning on different orientations with identical process conditions.

As stated previously, Fig. 5 is plotted using the metal work function, not necessarily the work function of the metal or metal oxide present at the metal–semiconductor interface that ultimately yields the electrical contact. As shown in the prior literature, oxidation does increase the work function of stoichiometric and non-stoichiometric metal oxides and may, at least partially, account for the non-unity values of S.30,31 Extracting the exact work function of these non-stoichiometric metal oxides is outside the scope of this study, except to note that their presence indicates an increase in the work function that may adjust ϕ B of metals, such as Ti and Cr (Fig. 4), to be aligned with the Schottky–Mott model. To further investigate oxidation as a source of non-ideal S values, we performed depth-resolved XPS measurements of the oxidation state of each contact metal at the contact- Ga 2 O 3 interface. The depth profiles are shown in Fig. 6. Despite all contacts not receiving a post-deposition anneal or thermal processing exceeding 200  °C for photoresist processing, the majority of the contact metals are at least partially oxidized. Due to the deposition occurring under ultrahigh vacuum pressures of 10 7 Torr, it is unlikely that the deposited metal was oxidized by oxygen during the line-of-site e-beam evaporation; oxidation is more likely due to a redox reaction with the underlying Ga 2 O 3.32 As expected, those metal oxides with the lowest free energy of formation at room temperature [i.e., Al 2 O 3, TiO 2, and Cr 2 O 3, Figs. 6(a)6(c)] show significantly more oxidation than the metal oxides with higher energy of formation [i.e., NiO, PdO, PtO 2, Figs. 6(d)6(f)].33 

FIG. 6.

Depth profiles of oxidation states of contact metals for (a) Al, (b) Ti, (c) Cr, (d) Ni, (e) Pd, and (f) Pt on β-Ga 2O 3 from decreasing to increasing energy of oxide formation. At room temperature, Ti and Cr are almost completely oxidized to TiO 2 and Cr 2 O 3, respectively, while Al, Ni, and Pd are partially oxidized to Al 2 O 3, NiO, and PdO, and Pt is entirely unoxidized.

FIG. 6.

Depth profiles of oxidation states of contact metals for (a) Al, (b) Ti, (c) Cr, (d) Ni, (e) Pd, and (f) Pt on β-Ga 2O 3 from decreasing to increasing energy of oxide formation. At room temperature, Ti and Cr are almost completely oxidized to TiO 2 and Cr 2 O 3, respectively, while Al, Ni, and Pd are partially oxidized to Al 2 O 3, NiO, and PdO, and Pt is entirely unoxidized.

Close modal

As the metals with the lowest ϕ M are also the metals that are most prone to oxidation and, therefore, most likely to experience an increase in the work function, the apparent Fermi-level pinning and low S values observed in metal Schottky contacts to Ga 2 O 3 may be attributed to under-reporting the work function of these oxidized and partially oxidized layers, in addition to any adverse effect that conventional processing may have introduced to the interface—most of the reports in the literature to date with the exception of Carey et al. and Cromer et al. have used a liftoff process. This could also explain the discrepancy between ϕ M and ϕ B observed for Pd and Pt, as the Pd layer is partially oxidized and may, therefore, have a higher work function than reported. Precise measurement and understanding of the value of the work function for partially oxidized and oxidized metal contacts is beyond the scope of this work. Future studies of barrier height extraction ought to be mindful of the significant influence of minute changes in E c relative to ϕ M from bandgap renormalization for accurate barrier height determination.

In conclusion, we report non-alloyed metal-first ohmic and Schottky contacts on β- Ga 2 O 3 with a range of contact metal work functions. We attain an ultralow contact resistance of 0.069 ± 0.003  Ω mm with Al contacts. Furthermore, we extract values for the Schottky-barrier height from the I–V characteristics of TLM patterns for the lower work-function metals and SBDs for the higher work-function metals. The extracted values of ϕ B largely increase with increasing ϕ M with an S value of 0.7 ± 0.2, indicating that the Fermi-level may at least somewhat be un-pinned by metal-first processing that preserves the bare-substrate ( 2 ¯01) and as-grown (010) surfaces in contrast with historical reports showing complete Fermi-level pinning on the ( 2 ¯01) and (010) surfaces. Depth-resolved XPS investigation of the oxidation state of the contact metals indicates that the majority of contact metals are at least partially oxidized even without alloying, which may result in higher work functions than reported and partially explain the persistence of apparent Fermi-level pinning. Further understanding of the crystal orientation dependence coupled with the precise effect of the oxidation state on work function may assist in further un-pinning the Fermi-level in β- Ga 2 O 3 and improving quality and consistency of Schottky and ohmic metal contacts.

See the supplementary material for additional sample growth details and processing details, an expanded discussion of Burstein–Moss and bandgap renormalization, illustrations of the criteria distinguishing between the TE and TFE regimes, details of the numerical tunneling model used to fit the reverse IV of the SBDs, and tabulated historical Schottky-barrier height measurements.

This work was in part supported by ACCESS, an AFOSR Center of Excellence (No. FA9550-18-1-0529). C.A.G. acknowledges support from the National Defense Science and Engineering (NDSEG) Fellowship. This work was supported in part by SUPREME, one of seven centers in JUMP 2.0, a Semiconductor Research Corporation (SRC) program sponsored by DARPA. The device fabrication was performed in part at the Cornell Nanoscale Facility, a NNCI member supported by NSF grant (No. NNCI-2025233). This work used facilities and instrumentation supported by the NSF through the Cornell University Materials Research Science and Engineering Center (No. DMR-1719875).

The authors have no conflicts to disclose.

Kathleen T. Smith: Conceptualization (lead); Data curation (lead); Formal analysis (lead); Investigation (lead); Methodology (lead); Validation (equal); Visualization (lead); Writing – original draft (lead); Writing – review & editing (equal). Cameron A. Gorsak: Investigation (supporting); Resources (equal); Writing – review & editing (equal). Joshua T. Buontempo: Investigation (supporting); Resources (equal). Bennett J. Cromer: Formal analysis (supporting); Visualization (supporting); Writing – review & editing (equal). Takumi Ikenoue: Funding acquisition (supporting); Supervision (supporting). Hemant Gulupalli: Investigation (supporting). Michael O. Thompson: Funding acquisition (equal); Supervision (equal). Debdeep Jena: Funding acquisition (equal); Supervision (equal). Hari P. Nair: Funding acquisition (equal); Supervision (equal). Huili Grace Xing: Conceptualization (equal); Data curation (equal); Formal analysis (equal); Funding acquisition (lead); Methodology (equal); Supervision (equal); Validation (equal); Writing – review & editing (equal).

The data that support the findings of this study are available from the corresponding authors upon reasonable request.

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