
Greater understanding of defect formation is needed to further increase the Curie temperature (TC) of ferromagnetic semiconductors, such as Ga1−xMnxAs, which hold promise for magnetoelectronic devices.1 In typical molecular beam epitaxy (MBE) growth of GaMnAs, low substrate temperatures (Tsub) of
250 °C are required to suppress precipitation of secondary crystal phases (e.g., MnAs) and incorporate a large fraction of Mn atoms as substitutional (MnGa) acceptors in GaAs. Mn atoms also form double-donor interstitials (Mni) that compensate holes. Annealing films in air at temperatures of
180 °C removes Mni,2 thus increasing the hole density (p) and TC, in agreement with the Zener model of carrier-mediated ferromagnetism.3,4 This model also predicts that TC increases linearly with MnGa, which is supported by studies over the past decade with 0.02<x<0.08.4 More recently, MBE growth of GaMnAs with x
0.1 was demonstrated in attempts to increase TC.5,6 These films require reduced Tsub (
180 °C) and are limited to
10 nm thickness; TC's after annealing reach the previous limit of
170 K.4 In these studies, the effect of arsenic flux was not explored, though it should be a critical parameter at these conditions.
GaAs films grown at Tsub
250 °C can contain double-donor arsenic antisites at concentrations AsGa
1020 cm−3 (
1% of Ga sites).7,8 For a fixed As:Ga flux ratio, AsGa in low-temperature (LT) GaAs increases exponentially as Tsub is decreased below
300 °C.9,10 Extended defects are prominent below 200 °C, leading to polycrystalline films.11,12 Previously, we developed combinatorial (nonrotated) growth to continuously vary As:Ga and, therefore AsGa, in GaMnAs films near the paramagnetic/ferromagnetic transition (
1% Mn) with Tsub=250 °C.13,14 There, excess arsenic flux of
1% suppresses ferromagnetism, an unfeasible flux precision for rotated growths. Here we extend this technique to Tsub
150 °C, where the metastable solubility limit of Mn in GaAs is increased beyond 10%. As in LT GaAs, increased AsGa and extended defects occur unless As:Ga is precisely balanced to achieve stoichiometry. We discuss systematic variations in magnetotransport, ferromagnetism, and crystal structure of GaMnAs (x
0.1) as As:Ga is varied along the [110] direction [Fig. 1(a) inset]. The highest TC's are obtained in a narrow band of stoichiometric material. Stoichiometric, 100 nm thick films exhibit excellent crystalline quality and square magnetic hysteresis up to 165 K. Stoichiometric films grown with varying x (>0.1), Tsub, and growth rate reach the same TC (150–170 K) after annealing; increasing MnGa does not increase TC as the Zener model predicts. We find that the linear dependence of TC on MnGa is limited to 0.02<x<0.1.
Figure 1. Samples are grown on 2 in., semi-insulating (001) GaAs wafers by MBE as described previously.13 The total fraction of Mn in the films (x) is calibrated from growth rate calibrations of MnAs and GaAs reflection high-energy electron diffraction (RHEED) intensity oscillations. After growth of the buffer layer, Tsub is dropped to 150 °C and substrate rotation is stopped. Below 350 °C, the arsenic shutter is closed; it is opened for 10 s prior to LT growth to ensure an arsenic-terminated surface. Tsub is measured in real time during growth using band-edge thermometry with an accuracy of ±2 °C.15 During the first 5–15 nm of growth, Tsub increases by
10 °C due to radiation from the heated Ga and Mn sources; Tsub quickly stabilizes after the heater power is dropped. We observe a two-dimensional (streaky) 1×2 RHEED pattern on As-rich material transitioning to a three-dimensional (spotty) pattern on Ga-rich material, observed by eye as a mirror finish (As-rich) transitioning to haze from Ga droplets on the surface.13 Wafers are cleaved into
3×3 mm2 pieces along [110], yielding
17 samples with systematically varying As:Ga.
Magnetometry and magnetotransport are measured on sample pairs with equal As:Ga (adjacent in the [
10] direction). Magnetotransport is measured in the van der Pauw geometry from 2 to 380 K with out-of-plane (hard axis) fields up to 14 T. TC is determined from superconducting quantum interference device (SQUID) magnetometry (Quantum Design magnetic properties measurement system SQUID vibrating sample magnetometer) while warming in 50 Oe ([110] in plane) after cooling from 350 K in 1 T. Saturation moment (Msat) is determined from hysteresis loops (<0.5 T). We anneal sample pairs in air at
180 °C until conductivity is maximized [Fig. 1(c) inset].2 High-resolution x-ray diffraction (HRXRD) is performed on half-wafers by using a triple-axis (Philips X'Pert MRD PRO) diffractometer with a 0.25° aperture for
1 mm resolution along [110]. Lattice constant (aGaMnAs) is determined from (004)
-2
scans.
Electronic, magnetic, and structural properties all depend critically on As:Ga. Figure 1 plots data from a single 100 nm thick Ga0.84Mn0.16As film grown with Tsub=150 °C at 0.852 Å/s. Room temperature longitudinal (
xx) and Hall (
xy) conductivities [Fig. 1(a)], TC and Msat at 5 K [Fig. 1(b)], and aGaMnAs [Fig. 1(c)] all maximize at the same As:Ga where stoichiometry is achieved.
xx increases with annealing [Fig. 1(c) inset] due to outdiffusion of Mni from the bulk to the surface.2 Examples of
-2
scans in Fig. 1(d) reveal high-quality XRD epilayer peaks with thickness fringes observed at stoichiometry (black points) which match dynamical simulations (line).16 The postannealing epilayer shift (red) shows a reduction in aGaMnAs from removal of Mni. This corroborates the model of Masek et al.17 and results of Sadowski and Domagala18 demonstrating that the main contributor to aGaMnAs expansion is Mni. It follows that the largest number of Mni occur for stoichiometric material, the same As:Ga at which TC, Msat,
xx, and
xy are largest.
As-rich material displays a broad XRD peak without thickness fringes, indicating low crystal quality [blue, Fig. 1(d)]. At this As:Ga, ferromagnetic MnAs particles (NiAs structure) are detected by magnetometry (TC=320 K). No remnant magnetization (Mrem) is observed at temperatures above the GaMnAs TC in the stoichiometric region, but a Mrem of 0.1µB/Mn from MnAs persists above the GaMnAs TC in the film with As:Ga=13.5 (35% greater than As:Ga=10, the stoichiometric condition). Excess arsenic might promote MnAs precipitation by creating extended defects that act as nucleation sites. MnAs is not observed in thinner As-rich films (7.5 nm), which could be below the critical thickness for defect formation. For our As-rich material, we reproduce previously observed limits5,6 to TC,
xx, and film thickness; these limits are overcome by achieving stoichiometry at precise As:Ga.
Excess arsenic and Mni significantly alter magnetic and electronic properties such as TC, Msat, coercive field (HC), resistivity (
xx), and magnetoresistance (MR). Figure 2(a) shows the TC increase to
165 K after minimizing defects, and we observe square hysteresis at this high TC [Fig. 2(b)]. Excess arsenic reduces the HC and Msat at 5 K [Fig. 2(c)].
xx and MR increase by orders of magnitude at 10 K in samples with Mni and excess arsenic [Fig. 2(d)]. Mni increases MR (at 14 T) from 3% to 44%, and excess arsenic (As:Ga=12) increases it to 87%.
xy switching occurs in all samples due to the anomalous Hall effect [Fig. 2(d)].
Figure 2. The growth parameter space of heavily alloyed GaMnAs is systematically explored with 16 nonrotated wafer growths with 0.1<x<0.22, 120<Tsub<160 °C, and growth rate varied from 0.198 to 1.41 Å/s. Figure 3(a) plots TC against x for the stoichiometric samples from each heavily alloyed wafer and also lightly alloyed wafers (x<0.1, 200<Tsub<250 °C). We observe the expected linear increase in TC with x (x<0.1),3,4 but it does not extend to the heavily alloyed regime, where TC=150–165 K postannealing for all x (maximum observed at x=0.16) despite the wide range of growth parameters. In contrast, aGaMnAs increases linearly up to x
0.16 for both as-grown and annealed films [Fig. 3(b)] and is fitted using the model of Masek et al.17,18 Assuming AsGa
0 in the stoichiometric region, aGaMnAs=aGaAs+0.02(x−z)+1.05z, where z is the atomic fraction of Mni and (x−z) is the atomic fraction of MnGa. Linear fits, plotted as lines in Fig. 3(b), demonstrate a constant fraction of interstitials (z/x) of 0.24 in as-grown samples and a reduction of this fraction to 0.13 after annealing. Recent theoretical work suggests that the coefficient for MnGa is larger than 0.02 (0.09), which would decrease our estimates of z/x.19 The linear behavior indicates that MnGa and Mni increase proportionally with x, up to x
0.16. Contrary to a prediction of the Zener model, TC is independent of x for x>0.1 even though Mni compensation maintains the same proportions in this heavily alloyed regime.
Figure 3. In conclusion, heavily alloyed, 100 nm thick GaMnAs films (0.1<x<0.22) with reproducible, high magnetic (TC
165 K), and structural quality are grown by utilizing a combinatorial technique to achieve stoichiometry. Magnetotransport, ferromagnetism, and lattice constant are critically dependent on As:Ga for low Tsub, with stoichiometric, annealed material displaying optimal properties. While structural and magnetic data indicate a linear increase in MnGa up to x
0.16, we do not observe the predicted TC increase,3 suggesting that the Zener model may not be applicable to the heavily alloyed regime. Application of this combinatorial technique provides a reproducible method for obtaining high-TC GaMnAs and allows systematic exploration of the growth parameter space.
We thank J. H. English and A. W. Jackson for MBE advice and M. A. Scarpulla for helpful discussions. This work was supported by ONR, MURI, and AFOSR. The authors used MRL Central Facilities supported by the MRSEC Program of NSF Contract No. (DMR05-20415). S.M. acknowledges support by the DoD through the NDSEG Fellowship Program.