The discovery of a two-dimensional electron gas (2DEG) at the interface between two insulators LaAlO3 (LAO) and SrTiO3 (STO)1 has not only enhanced the expectations in oxide-electronics but has also brought new and exciting opportunities to explore the novel physics of 2DEG with unmapped parameters. In recent years, this interface has been studied extensively and several exotic phenomena including superconductivity,2,3,4 Rashba spin-orbit coupling,5,6,7 ferromagnetism,8,9,10 and quantum oscillations11,12,13,14 have been reported. The leading consensus for the formation of the 2DEG at this interface is the electronic reconstruction (also referred to as the “polar catastrophe").15,16 This scenario is based on electron transfer from the polar LAO to the interfacial layers of STO, although other mechanisms such as oxygen vacancy doping17,18 or interdiffusion19 are also at play.

First-principles calculations of the band-structure reveal the occupancy of several non-degenerate sub-bands dxy, dxz and dyz originated from crystal field splitted Ti:3dt2g orbitals located at the interface or in its vicinity.20 Using combination of k.p envelope function method and density functional theory, Heeringen et al.21 confirmed the existence of many anisotropic and non-parabolic sub-bands, which are only a few meV apart. Meanwhile, Zhong et al.6 predicted a large spin-orbit splitting at the crossing point of the dxy and dxz∕yz bands using density functional theory. To date, the predicted band-structure has received only partial support from transport experiments. Indeed, the analysis of Shubnikov-de Haas Oscillations (SdHO) provided distinctive results with respect to different experimental conditions and sample preparation methods. In refs,11,12 the authors reported independently a single SdHO frequency and pointed out the possible valley and/or spin degeneracy of the electronic states to account for the discrepancy between the carrier density extracted from the SdHO and the Hall effect. Later, double SdHO frequencies perceived up to a moderate magnetic field (8 T) and at low temperature (50 mK) were attributed to carriers populating the heavy sub-bands dxz and dyz splitted by the Rashba spin-orbit interaction.22 On the other hand, McCollam et al.13 extracted four frequencies using high magnetic field (20 T) for the SrTiO3/SrCuO3/LaAlO3/SrTiO3 hetero-structure, and assigned these frequencies to four sub-bands of different mobilities. In contrast, very high field (55 T) measurements reveal quasi-1/B periodic oscillations with an apparent single frequency, which emphasizes the role of Rashba spin-orbit interaction.14 No consensus is reached in the interpretation of the magneto-transport properties and further work is needed to enrich the debate. In addition, it is worth mentioning that a systematic discrepancy between the carrier density estimated from Hall effect (nHall) and SdHO (nSdHO) is reported by several groups.11,12,14

Here, we investigate the transport properties of a high mobility (μ > 104 cm2 V−1 s−1) 2DEG at the LAO/STO interface under very high magnetic field (55 T) and low temperature (1.6 K). We observe strong 1/B-aperodic SdHO where the frequency increases with magnetic field. The hypotheses leading to this unexpected effect are discussed below, after reviewing the experimental data.


The sample under investigation consists of 8 unit cells of LAO grown on top of a 500 μm STO (001) substrate using a pulsed laser deposition technique at the temperature of 760 °C and in 2 × 10−6 Torr oxygen pressure. After the LAO growth, the sample is annealed in 6 × 10−2 Torr oxygen pressure at a temperature of 600 °C to remove oxygen vacancies. High Resolution Scanning Transmission Electron Microscope (HRSTEM) analysis reveals a mono-crystalline LAO layer without surface roughness while a large cation intermixing extends within two-three unit cells from the interface in both LAO and STO. The lattice spacing is expanded of about 5.5% along the growth axis, however no distortion is observed in the growth plane. The sample is tailored into a Hall bar of width 50 μm and length 160 μm (see Supplementary information 1). Both the longitudinal magneto-resistance (Rxx) and the Hall resistance (Rxy) are measured simultaneously during a pulse of magnetic field up to 55T at a temperature T = 1.6 K. Such measurements are repeated for several values of back-gate voltage Vg, which is applied at the rear face of the STO substrate to modulate the carrier density of the 2DEG. The panels a and b of Fig. 1 show the magnetic field dependence of Rxx and Rxy, respectively, recorded at different back-gate voltages from 0 to −15.5V. The depopulation of the 2DEG leads to a substantial increase in zero-field resistance as well as an increasing positive magneto-resistance. In contrast, the longitudinal and Hall resistances change marginally as the back-gate voltage is set at positive values in the range ~5–60 V as shown in Fig. 1d, e. After subtracting the monotonic background (see Supplementary Information 2), we show ΔRxx(B) = Rxx(B) − 〈Rxx(B)〉 for various Vg in Fig (c) and (f), respectively. While the position of the extrema in ΔRxx(B) spectra shifts significantly towards a lower magnetic field for negative back-gate voltages, a slight deviation is noticed above Vg ~ 5 V, which reflects a saturation of the carrier density.

Fig. 1
figure 1

Left panels: magnetic field dependence of (a) Rxx, (b) Rxy and (c) ΔRxx for different values of Vg in the range 0 → −15.5 V. Right panels: magnetic field dependence of (d) Rxx, (e) Rxy and (f) ΔRxx for different values of Vg in the range 5 → +60 V. The temperature is 1.6 K. ΔRxx is the oscillating part of Rxx after extracting the monotonous background. A significant back-gate induced shift in the position of the ΔRxx oscillations extrema is observed only for Vg < 5 V. Above this value, the oscillation pattern is almost unchanged concurrent with the saturation of nHall(Vg).

The Hall carrier concentration (nHall) estimated from the slope of the linear fit of Rxy(B) and mobility (μHall) are plotted versus Vg in Fig. 2. Taking into account the electric field dependence of the STO dielectric constant,23 the plane capacitor model (Supplementary Information 3) reproduces well the experimental Hall carrier density in the back-gate voltage range −7 V < Vg < 5 V. For negative back-gate voltages, the mobility decreases due to the enhanced electron’s sensitiveness to emerging local potential fluctuations. Indeed, as the carrier density becomes low, screening of charged defects in the close environment of the 2DEG vanishes, leading to a rise of the scattering rate. For Vg < −7 V, the Hall voltage shows large temporal fluctuations and eventually becomes unmeasurable (see dotted-lines in Fig. 1(b)), as if the sample was turn into an insulator. This reversible trend is confirmed by Rxx which abruptly exceeds the measurement limit (~1 MΩ) for Vg < −15.5 V. In this regime, i.e., when the Hall 2DEG carrier density is below the threshold value of ~0.98 × 1013 cm−2, electron localization arises successively in different locations of the sample, leading to a transport regime governed by the presence of percolating conduction paths. This scenario, in agreement with the direct visualization of sub-micrometer electron puddles using scanning SQUID spectroscopy24 and inter-modulation electrostatic force microscopy,25 provides a natural explanation for the apparent mismatch between Rxx and Rxy back-gating insulating thresholds. On the other hand, when the back-gate voltage is pushed beyond +10 V, the Hall carrier density saturates to a maximum value of ~1.95 × 1013 cm−2. This response is accompanied by a strong hysteretic behavior, which originates from the trapping of electrons by defects.26,27 Indeed, assuming that the 2DEG is confined in a potential well close to the interface with the Fermi energy lying close to the top of the well, a positive back-gate voltage modifies the well profile and bends the STO conduction band. As a consequence, electrons can irreversibly escape the well and get trapped by defects. Interestingly, the carrier density can be reset to its Vg = 0 V initial value (after a round trip to +60 V at 1.6 K) by warming up the sample slightly above 20 K. We thus infer a very small average trapping energy of the order of 2 meV in our sample. We conjecture that the growing number of ionized defects, acting as remote scattering centers, is responsible for the variation of the Hall mobility which decreases simultaneously with the onset of carrier density saturation. Oxygen vacancies are often cited as potential defects in oxides but, eventhough investigations on the nature of the defects is certainly beyond the scope of this study, we believe that they are not at play in the electron trapping process. Indeed, first we remind that our sample was annealed in oxygen atmosphere and the resulting carrier density is lower than that typically obtained from the LAO/STO interfaces prepared in a low oxygen partial pressure without a subsequent high pressure post-annealing. Second, the oxygen vacancies are positively charged when they transfer one or two electrons to the 2DEG. The capture of electrons with increasing back-gate voltage would render them neutral, which is inconsistent with the experimentally observed mobility decrease. The main panel of Fig. 3a focuses on the inverse magnetic field dependence ΔRxx for Vg = 0 V. We notice that the frequency of the oscillations increases monotonically with increasing magnetic field in our LAO/STO sample. This unexpected effect becomes clearer in the Landau plot, where the extrema of the oscillations are plotted as a function of 1∕B in the inset of Fig. 3a. Interestingly, the Landau plot is highly nonlinear, contrary to the standard 2DEG in semiconductor heterostructures or in graphene. As a matter of fact, the SdHO aperiodicity was apparent in the early literature of quantum transport in LAO/STO systems above 1 K.11,28 However, this evidence has probably been overlooked due to the narrow magnetic field range and limited number of oscillations. Similarly, δ-doped STO also exhibits aperiodic oscillations up to Bmax = 15 T in reference.29 Our magneto-resistance data could certainely be fitted using an appropriate combination of 1/B-periodic signals, referring to a complex set of unresolved sub-bands in the experimental conditions of temperature, magnetic field and samples’ mobility. Although this multi-band model cannot be a priori discarded, the smooth evolution of the oscillating features call for alternative interpretations. In the following, we discuss different possible scenarios that can lead to the 1/B-aperiodic SdHO, while keeping in mind that due to the limited number and the poor low-field resolution of the observed oscilllations, the apparent 1/B-aperiodicity may or may not have an intrinsic origin.

Fig. 2
figure 2

a Charge carrier density estimated from the Hall resistance (green symbols) and the plane capacitance model (red solid line). b Electron mobility estimated from the Hall density and the zero-field longitudinal resistance. The dash lines are guides for the eyes. The region between two vertical dotted lines (−7 V < Vg < 10 V) indicates a reversible back-gate induced electron density modulation. The right side of the vertical line represents an hysteretic charge trapping/detrapping regime by ionized defects, leading to a saturation of the carrier density. The inset depicts an illustration of the LAO/STO interface including confining potential and electron trapping process.

Fig. 3
figure 3

a Main panel: Inverse field dependence of ΔRxx for Vg = 0 V. Inset: the corresponding Landau plot. Maxima and minima of ΔRxx(1∕B) are assigned to integer and half-integer indices, respectively. b Landau level plots (symbols) for Vg = 0 V, −10 and −15.5 V fitted with Eq. (3) (solid lines). The dash line represents the asymptote for Vg = 0 V derived from the fitting parameters F(μ,0) and γ(μ,0)—See also Table 1. The index N is given within an integer offset \((N^{\prime} )\).


When plotted as a function of inverse magnetic field, the frequency \(F=\frac{h.S}{{\left(2\pi \right)}^{2}.e}\) of the magneto-resistance oscillations is proportional to the area in the reciprocal space of the cyclotron orbit S, which obeys the Onsager’s quantization condition:

$$S=\frac{{\left(2\pi \right)}^{2}\,e\,B}{h}\times \left(N+\frac{1}{2}\right)$$

Here h and e are respectively the Planck constant and the electron charge, and N is a positive integer index related to the formation of Landau levels. S is linked to the carrier density nSdH and to the topology of the Fermi surface. Taking into account the total degeneracy (g = gs.gv) of the quantum states, these parameters set the Fermi energy EF (e.g., the chemical potential μ, assuming low enough temperature). To explain the continuous increase of the frequency F as the magnetic field rises, we are left to question (i) the quantization rule itself as well as the possible magnetic field dependence of (ii) EF and (iii) nSdH.

The scenario (i) is met when the quantization of the electron’s kinetic energy results from a competition between the electrical and the magnetic confinement. This route has been recently explored by G. Cheng et al.30 who studied the conductance of an individual and artificially designed quasi-1D conduction channel at the LAO/STO interface. The model, derived from,31 predicts an alteration of the oscillations’ frequency which can merely fit our experimental data (see Supplementary Information 4). However, this approach must be adapted to the quasi-2D nature of our sample by considering the presence of an incoherent network of quasi-1D channels at the interface. Even if this hypothesis may find an echo with the formation of percolation paths at low carrier density, or with the presence of grain boundaries acting as potential wells, the origin of the quasi-1D channels remain strongly elusive.

The hypothesis (ii) refers to a magnetic field-induced change of the Fermi surface topology, while the carrier density is kept constant. In this scenario, the chemical potential of the system is allowed to change as the magnetic field affects the electron’s dynamics. In pure 2D systems, a constant carrier density necessarily implies a fixed frequency for the Shubnikov-de Haas oscillations, regardless any eventual variation of the chemical potential or Fermi surface topology. This is because the kinetic energy of the electrons is affected by the (perpendicular) magnetic field and must fit into Landau levels. Therefore, the 1/B-periodic magnetic oscillations results from the filling of a fixed number of electrons into Landau levels, whose degeneracy is strictly proportional to the magnetic field. This picture, however, no longer holds if one introduces other energy scales due to spin-orbit coupling, Zeeman effect and disorder. Indeed, the Landau level energy ladder can be strongly modified, ensuing the formation of new energy levels with different effective degeneracy.14,22 In particular, Trier et al.28 pointed out a Zeeman energy gμB. B comparable to the orbital Landau level gap ħeBm* for large effective mass (m* ~ 1.3 × me) in LAO/STO. This model predicts an unusual magnetic field doubling of the oscillation’s frequency corresponding to the transition from a spin-degenerate to a spin-resolved Landau level ladder. We note, however, that the Zeeman effect alone cannot explain our experimental results since the frequency of the oscillations is actually multiplied by 3.6 (e.g., larger than 2) from 12 to 34 T. Rashba spin-orbit coupling certainly affects the topology of the Fermi surface and consequently the periodicity of the quantum oscillations. Based on the work of Fete et al.,22 Yang et al.14 have discussed this scenario to explain the quasi 1/B-periodic nature of the oscillations in the same system. However, we could not fit our present data (with larger aperiodicity) using this model. We note that the Rashba effect is certainly oversimplified in this model, and a more accurate description requires advanced and dedicated calculations which are out of the scope of the present manuscript. In contrast, deviations from strictly 1/B-periodic oscillations are well known in 3D systems for small Landau level indices.32 This effect is however too weak to compare with our experimental observations, provided the electron gas at the LAO/STO interface can be regarded as a (quasi)-3D system. In the context of a fixed number of electrons, a deformation (reconstruction) of the Fermi surface, eventually driven by the Coulomb interaction, is likely to trigger a field-induced Lifshitz transition. However, we expect this phenomenon to translate into a sharp signature in the magneto-resistance at a certain value of the magnetic field in contrast with the smooth evolution of the oscillation’s frequency and amplitude.

The assumption (iii) considers the case of a variable carrier density while the chemical potential is kept constant. Similar to graphene on silicon carbide,33,34 one possibility is to infer that electrons are continuously transferred from a nearby reservoir to the LAO/STO interface as the magnetic field increases. Although this model sounds attractive, it relies on a hypothetical charge reservoir with strong capacitive coupling to the 2DEG, so that the quantum capacitance of the system drives the charges’ dynamics. To our knowledge, we are not aware of any charge reservoir in the vicinity of the LAO/STO interface and this hypothesis is therefore discarded. On the other hand, inspired by the recent work of Gao and Niu,35 who introduced a generalized Onsager’s relation to explain the 1/B-aperiodic quantum oscillations observed in systems with complex topological order, we now consider an alternative approach involving the magnetic response functions of the system. Following the lines of Fuchs et al.,36 the averaged carrier density 〈n〉 derives from the derivative of the grand potential Ω(μ,B) with respect to the chemical potential μ, which is itself expanded in Taylor series with respect to the magnetic field:

$$\langle n\rangle =-\frac{1}{S}\frac{\partial }{\partial \mu }\left({\Omega }_{(\mu ,B)}\right)=-\frac{\partial }{\partial \mu }\left(\frac{1}{S}{\Omega }_{(\mu ,0)}-{m}_{0}\times B-\frac{{\chi }_{{}_{0}}}{2}\times {B}^{2}+...\right)$$

where \({m}_{0}=-\frac{1}{S}\frac{\partial }{\partial B}\left({\Omega }_{(\mu ,0)}\right)\) and \({\chi }_{{}_{0}}=-\frac{1}{S}\frac{{\partial }^{2}}{\partial {B}^{2}}\left({\Omega }_{(\mu ,0)}\right)\) are the averaged magnetization and magnetic susceptibility at zero field, respectively. Combining Eqs. (2) and (1) and setting \({n}_{0}\equiv -\frac{1}{S}\frac{\partial }{\partial \mu }\left({\Omega }_{(\mu ,0)}\right)\) one obtains:

$$N={F}_{(\mu ,0)}\times \frac{1}{B}-{\gamma }_{(\mu ,0)}+{C}_{(\mu ,0)}\times B+...$$

where F(μ,0) is the frequency of the oscillations at low magnetic field, e.g., the slope of the Landau diagram asymptote for 1∕B. The coefficient \({\gamma }_{(\mu ,0)}=\frac{1}{2}-\frac{\partial {m}_{0}}{\partial \mu }\) sets the phase of the Shubnikov-de Haas oscillations and corresponds to the intercept of asymptote for 1∕B with the index axis in the Landau plot. Finally, the coefficient \({C}_{(\mu ,0)}=\frac{h}{4.e}\frac{\partial \chi _{{}_{0}}}{\partial \mu }\) is linked to the curvature of the Landau plot. Table 1 reports the best fitting parameters F(μ,0), γ(μ,0) and C(μ,0) determined from the fit of the experimental data (this work and literature—Supplementary Information 5) to Eq. 3, as well as the Hall carrier density (nHall) and the SdHO carrier density (\({n}_{SdH}=\frac{2.e}{h}{F}_{(\mu ,0)}\)) for comparison.

Table 1 Parameters determined from the fit of the Landau plot.

Interestingly, all the parameters exhibit a monotonous evolution with gate voltage (see Supplementary Information 6). While F(μ,0) and γ(μ,0) from high (55 T—this work) and low field (12 T—refs 11,28) experimental data are of the same order of magnitude, a fair discrepancy occurs in C(μ,0) for different field regimes and carrier density. The variance of C(μ,0) can be explained by (i) different carrier density, (ii) different levels of disorder, and (iii) magnetic field range over which the fit is performed. It is actually worth mentioning that the accuracy of the fit parameters is restricted by the limited number of oscillations, especially at low field. Even if the recent observation of non-zero magnetic response functions3,9,37 of the LAO/STO interface and the expected enhanced susceptibility in the low-electron-density regime38 are in line with the non-linear Landau plots, improved precision on γ0(E) and C(E) is needed in order to obtain a quantitative agreement.

The cases (ii) and (iii) are certainly an idealization of real systems, where both the charge carrier concentration and the chemical potential may indistinguishably vary. The combined effects translate into a change of S as a function of the magnetic field, whose relative increase reaches up to 1000% in the 0–55 T magnetic field range, assuming a zero-field electron density of 1 × 1012 cm−2 (See Supplementary Information 7). At first sight, the linear Hall effect tends to favor a scenario with a constant carrier density. However, this claim must be taken with care since a quasi-linear Hall effect is allowed in a multi-carrier system with fixed total charge density. A magnetic field-induced transfer of electrons from low-mobility to high-mobility bands is indeed compatible with an increase of the quantum oscillations’ frequency, while the Hall coefficient is only weakly affected. It is worth to mention that the non-trivial band-structure of the LAO/STO interface at the Fermi energy may also generate aperiodic oscillations in high field regime similar to the non-ideal Dirac fermion systems.39

The hypothesis (iii) provides a new approach to compute the carrier density from aperiodic oscillations which was otherwise systematically over-estimated using fast Fourier transform (FFT) analysis. Indeed, the strong aperiodicity tends to broaden the FFT spectrum towards high frequency and can even favor the onset of spurious FFT peaks when the magnetic field range is extended towards very high magnetic field (see Supplementary Information 8). To complement this insight, we revisit the large discrepancy between nHall and nSdHO using density functional theory (DFT) calculations, where the density of states projection of the dxy and dxzdyz subbands at the Fermi energy is investigated. The layer-resolved density of states with electronic band structure of the LAO/STO interface are shown in Fig. 4. The lower lying dxy subbands (1dxy and 2dxy) are populated by a majority of electrons located mainly into the first two TiO2 planes from the interface. On the other hand, dxz/dyz subbands are populated by a minority of electrons whose spatial extension expands from the second to the sixth TiO2 plane. Based on HRSTEM analysis, we conjecture that cation intermixing, strain and probably the non-homogeneous valence of the titanium atoms generate potential fluctuations in the two first layers of STO at least, which strongly affect the electronic mobility. Therefore, the majority of electrons belonging to the 1dxy and 2dxy subbands will have low mobility even if they display low effective mass and do not engender quantum oscillations. They contribute mainly to the linear Hall effect with a theoretical carrier density estimated to \({n}_{{d}_{\mathrm{xy}}}\approx 6\times 1{0}^{13}\) cm−2. The SdHO ensue from the minority charge carriers located deeper in STO and belonging to the higher energy dxz/dyz subbands. The cyclotron mass, mc = 1.75 + 0.05me estimated from the Lifshitz-Kosevich equation fitting (see Supplementary Information 9) is consistent with the theoretically calculated averaged effective mass (m* ~ 1.8me) of the dxz/dyz subbands. The theoretical carrier density for these subbands is estimated to \({n}_{{d}_{xz/yz}}\approx 5.2\times 1{0}^{12}\) cm−2 taking into account the fourth, fifth, and sixth layers where the density of state projection of the dxz/dyz subbands is relevant. Even if the DFT based model does not reflect a realistic LAO/STO system (for instance the presence of defects is not taken into account and the exact position of the Fermi energy is unkown), this study shows that a large ratio of nHall and nSdH (nHallnSdH ~ 13 − 18 from Table 1) observed experimentally can be conveniently explained by the relative population of the dxy, dxz and dyz subbands, where \({n}_{{d}_{\mathrm{xy}/\mathrm{xz}/\mathrm{yz}}}/{n}_{{d}_{\mathrm{xz}/\mathrm{yz}}}\) approches ~14.

Fig. 4: Left panel: The layer-resolved density of states (LDOS) in LAO/STO.
figure 4

Each LDOS corresponds to a AlO2 or TiO2 plane. The black curve corresponds to the total LDOS of the TiO2 plane, the blue, green and red curves correspond respectively to the dxy orbital, the dyz + dxz orbitals of Ti and the 2p states of oxygen. Right panel: Electronic band structure of the STO in LAO/STO system. Inset shows a zoomed-in view of band avoiding and splitting due to the atomic and Rashba spin-orbit coupling.

The magneto-transport properties of a high-mobility electron gas at the LAO/STO interface are studied under high magnetic field (55 T) and low temperature (1.6 K) for different carrier densities. We observe 1∕B-aperiodic SdHO over the full magnetic field range (9–55 T). The aperiodic character of the oscillations involves the failure of standard FFT data processing, unless the analysis is restricted to low enough magnetic field. Pre-empting the fact that only very low temperature combined with high-field measurements are necessary to address the extrinsic (multi-band) origin of the measured 1∕B-aperiodic oscillations, we explore several alternative scenarios which provide new insights and bring further evidence for a non-trivial band structure at the Fermi energy, in consistency with DFT calculations where dxy, dxz and dyz subband anti-crossings occur due to spin-orbit coupling. When the Fermi energy is located in the vicinity of the dxzdyz subbands bottom, a fair correspondence can be established between electrons’ location within the TiO2 planes and the subbands to whom they belong. The majority electrons populating the dxy subbands are located close to the interface and are sensitive to interface disorder as revealed by HRSTEM analysis. Their low mobility and high carrier density explain the linear field dependence of the Hall resistance. On the other hand, the minority of charge carriers belonging to the dxz/dyz bands and located deeper from the interface are responsible for the SdHO with strong aperiodic behavior. In this scheme, the long-standing issue regarding the mismatch in carrier density extracted from the Hall effect and the SdHO finds a qualitative explanation, based on the sample’s dependent relative population of the dxz, dyz and dxy subbands.


Sample fabrication and structural characterization

The 8 unit cells of LaAlO3 film were grown on a TiO2-terminated (001) SrTiO3 single crystal using pulse laser deposition (PLD) technique at NUSNNI-Nanocore National University of Singapore (NUS). The Lambda Physik Excimer KrF UV laser with the wavelength of 248 nm at a pulse rate of 1 Hz was used in PLD. The layer-by-layer growth of LaAlO3 was precisely controlled by in situ reflection high energy electron diffraction (RHEED). During growth, the oxygen partial pressure \({P}_{({O}_{2})}\) and temperature were maintained at 2 × 10−6 torr and 760 °C, respectively. After growth, the sample was cooled down to room temperature at a rate of 5 °C/min with same \({P}_{({O}_{2})}\). Later, the sample was annealed in the \({P}_{({O}_{2})}\) of 60 mtorr and at the temperature of 600 °C. The six-terminal Hall bar device of width 50 μm and length 160 μm between the longitudinal voltage leads was fabricated by conventional photolithography technique using AlN films as hard mask. The optical microscopy image of the Hall bar device is shown in the Supplementary Information 1. The cross-section of the LAO/STO structure was characterized using a probe Cs-corrected JEOL JEM-ARM200F Transmission Electron Microscope (TEM) operated at 200 kV at CEMES. Focused ion beam was used to prepare the TEM lamella.

Transport measurements

The transport measurements under high magnetic field and low temperatures were carried out at Laboratoire National des Champs Magnétiques Intenses (LNCMI) Toulouse. For transport measurements, the device was electrically bonded with Al wires using wedge bonding. The sample was cooled down from room temperature to 1.6 K with a cooling rate of ~3 K/min in a He4 cryostat. The sheet resistance decreases from 250 kΩ to 130 Ω as the temperature is decreased from 300 K to 1.6 K. The simultaneous measurements of longitudinal and Hall voltages were performed under high pulsed magnetic field of up to 55 T with duration 300 ms and at T = 1.6 K. The back-gate voltage was varied from 0 to −15.5 V and from 0 to 60 V for tuning the carrier density at the interface. The dc current excitation was 1 μA. All magneto-transport measurements were performed with the magnetic field oriented perpendicular to the sample’s plane.

First-principles calculations

The ab initio calculations have been performed using the plane wave code VASP40,41 and the generalized gradient approximation (GGA)42 for the exchange-correlation energy. More details are given in the Supplementary Information 10.