Curie temperatures of the concentrated and diluted Kondo-lattice model as a possible candidate to describe magnetic semiconductors and metals

Curie temperatures of the concentrated and diluted Kondo-lattice model as a possible candidate to describe magnetic semiconductors and metals

M. Stier\Ast,1 and W. Nolting1 1Festkörpertheorie, Institut für Physik, Humboldt-Universität, 12489 Berlin, Germany

We present a theory to model carrier mediated ferromagnetism in concentrated or diluted local moment systems. The electronic subsystem of the Kondo lattice model is described by a combined equation of motion / coherent potential approximation method. Doing this we can calculate the free energy of the system and its minimum according to the magnetization of the local moments. Thus also the Curie temperature can be determined and its dependence on important model parameters. We get qualitative agreement with the Curie temperatures’ experimental values of GaMnAs for a proper hole density.

Kondo-lattice model, diluted magnetic semiconductors, correlated electrons


1 Introduction

Ferromagnetism is a solid state phenomenon which arises from the interplay of magnetically active atoms or their electrons, respectively. Naively one would think that high Curie temperatures are connected to a high density of those atoms. Thus it was suprising when relatively high Curie temperatures[1, 2, 3] in diluted magnetic semiconductors (DMS) with over 100K were discovered - even at small amounts of magnetic atoms. This finding and the high spin polarization of the carriers made the DMS a possible candidate for spintronic devices[4]. It is a major task to understand these materials and thereby improve them to eventually achieve room temperature magnetism.
One prominent DMS is GaMnAs which has a up to K for a concentration of of manganese ions[5]. Manganese, which replaces dominantly gallium, has a partly filled -shell, in contrast to gallium’s completely filled -shell. To calculate the effect of this doping several methods can be used. Ab-initio calculations are able to calculate the full density states of a specific material. This gives insight into the position of the impurity levels within the bulk material. Additionally Curie temperatures of different DMS can be calculated accurately[6, 7]. Besides ab-initio methods, model studies are useful to find the main mechanism which leads to ferromagnetism in DMS. For GaMnAs the -states of manganese lie deep below the valence band[4, 6] of the host material and are therefore assumed to lead to a localized spins at the impurity site with spin quantum number . Although the states are deep below the Fermi level they can interact with carriers (holes) in the valence band which influences its band structure. This results in an effective exchange between the localized spins (even though they are far away from each other at strong dilutions) which can lead to ferromagnetic order.
One of the major problems is to have control over the carrier density ( for electrons or for holes). Nominally one manganese ion provides one hole but due to compensation effects the ratio is usually smaller than one. As the mean-field Zener model predicts this seems to reduce the Curie temperature. In contradiction experiments show[8, 9] that a hole compensation is rather necessary for a finite . The same is true for theoretical approaches beyond the mean-field approximation[10, 11, 12]. To calculate the Kondo lattice model (KLM) is often mapped onto a Heisenberg model, which is then solved with different approximation methods. Contrary to that we propose a procedure how to calculate the free energy exclusively from the electronic subsystem so that we get the Curie temperature directly from the KLM.
The paper is organized as follows. First we introduce the model Hamiltonian. After that we describe how we calculate the internal energy of the system by an equation of motion approach. In the case of a diluted system we combine that with a coherent potential approximation. As the next step we use the internal energy to get the free energy where we also need the entropy at K. From the free energy we calculate Curie temperatures in dependence of several model parameters. These are compared with experimental data.

2 Model

We use the Kondo lattice model to describe the interactions between local moments and itinerant conduction electrons with spin , with the standard Hamiltonian


The itinerant electrons, represented by the creators (annihilators) , move from lattice site to due to the hopping . They prefer to align parallel () or antiparallel () to the local moment on the same site.
In the context of DMS the localized moments are formed by the -states of the magnetic impurities while the itinerant carriers move in the valence band (holes) or in the conduction band (electrons). In GaMnAs the hole created by the replacement of Ga with Mn is within the three antibonding -levels with dominant As 4p character[4]. This actually requires a multiband treatment but to simplify the calculations the valence band is approximated in a one-band model. The conduction band is completely neglected.
Since the magnetic impurities are randomly distributed within the host material we have to include disorder to our model. This is done via an introduction of a random variable indicating if a magnetic impurity is present at lattice site . The concentration of the magnetic atoms is fixed by the requirement . Besides the magnetism of the impurities there can be other effects on the electrons[13, 11], e.g. different atomic levels for magnetic (M) and non-magnetic sites (NM). We choose while may be unequal zero. We end up with the Hamiltonian


where we wrote the scalar product in (1) with the help of Pauli matrices and explicitly. There is now an Ising term (, ) and a spinflip part (, ).
Since our model is not restricted to small doping we are able to calculate the whole range to show general trends of the influence of dilution.

3 Electronic part

In this work the key quantity is the internal energy . It can be derived in the KLM from the single-electron Green’s function (SE-GF)


with the thermodynamic average and the usual step function . Operators are in the time dependent Heisenberg representation. The GF can be Fourier-transformed to its energy representation


In the KLM the internal energy then is simply given as


where the Fermi function contains the chemical potential and the inverse temperature . Thus, to calculate , we need to find an expression for . In a first step this will be done for the concentrated lattice () and then will be extended to diluted lattices.

3.1 Single electron Green’s function in the concentrated lattice

To get the SE-GF we will perform a moment conserving decoupling approach (MCDA[14]) of higher Green’s functions appearing in several equations of motion (EOM). Let us start with the EOM of , which reads


We can introduce a self-energy


which leads, after Fourier transformation, formally to the solution


The commutator in (7) can also be calculated explicitly, yielding


with the reduced Ising function and the spinflip (SF) function . These functions can also be calculated by their EOMs. Within these equations we treat diagonal () and non-diagonal terms () differently. For the non-diagonal elements we replace approximately


as in Eq. (7), which is only strict for , of course. As an example:


The higher Green’s function is therewith traced back to a linear combination of Ising functions. It is easy to see that the functions on the left- and the right-hand side have the same pole structure differing only by the respective spectral weights. The latter is approximately compensated by a self-consistent determination of the expansion coefficients which are just the elements of the central self-energy matrix. Higher Green’s functions with commutators containing only spin operators (e.g. ), are neglected, since they scale with magnon energies which are much lower than those of the electrons[14]. The commutators of the diagonal terms, however, are calculated explicitly which leads to further Green’s functions , where stands for different combinations of spin and electron operators. These functions can be expressed in some limiting cases (e.g. , , or ) rigorously by the three Green’s functions mentioned above suggesting the general ansatz


which we approximate to be valid for all parameter constellations. The prefactors are fixed by the requirement of conservation of the first spectral moments of the Green’s functions and their according expectation values. Since the moments are conserved we then get a correct high energy behavior of these functions[15, 16].
After performing the mentioned approximations we get unique solutions for the Ising- and spinflip Green’s functions (details in Ref.[14]). These can be written in the form


and we see that they are proportional to the one-electron Green’s function. This allows us, by comparing Eqs. (6, 7) and (9), to identify the prefactors in (15) with the self-energy


which splits into a mean-field and a more complicated ”many-body” part. The latter is defined by the , which depend on several expection values. These either contain only spin operators or also electronic operators. The ”pure spin operator” values (e.g. ) can all be expressed by the well known formula of Callen[17] as functions of the local moment magnetization . To do this we implicitly assume that a mapping of the KLM onto a Heisenberg model is in principle possible, but we do not have to perform it explicitly. All other expectation values (e.g. , , ) can be calculated with the spectral theorem from the known Green’s functions , and . But the do not only depend on scalars but also on the local Green’s function and the self-energy itself. These dependencies necessitate a self-consistent calculation of the self-energy.
Especially the dependence on the local Green’s function


will play a crucial role when we consider diluted systems.
Since we want to focus on the interaction of local moments and carriers, we have neglected a direct influence of the Coulomb repulsion in the conduction band. An addition of that would be especially necessary to describe narrow band materials like the manganites[18]. The inclusion of a Hubbard-type Coulomb term could lead to extra effects in magnetic ordering (band-magnetism), which are not accounted for in this work.

3.2 Single electron Green’s function in the diluted lattice

The diluted KLM can be described as a binary alloy. The components are defined by the sites with or without magnetic impurities. In the coherent potential approximation (CPA[19]) the configurationally averaged Green’s function of the total system is given by


The CPA self-energy can be derived self-consistently from


As the concentration of the magnetic impurities is a parameter we only need to determine the potentials to solve the problem. We set for the non-magnetic sites. For the magnetic sites we choose the self-energy (16) as an energy dependent potential (dynamical alloy analogy, DAA[20, 10]). In Section 3.1 we calculated the self-energy , put it into formula (8) to get and calculate again until self-consistency is achieved. But we have to keep in mind that the self-energy was derived for a concentrated lattice. In a diluted system the magnetic component is embedded in the total system. Thus we change the self-consistency cycle a bit.
Since the main change of the Hamiltonian (2) for the diluted system is only the inclusion of scalar random variables , we assume that the equations of motion of the magnetic subsystem have the same formal structure as in Section 3.1. That means especially that the self-energy is a function of the local Green’s function (Eq. (17)). As we want to calculate only the self-energy of the magnetic subsystem it should only depend on the local Green’s function of this subsystem. Thus we replace in Eq. (17) yielding


where is the magnetization of the impurity system. The subsystem’s Green’s function of component can be calculated via the projection[19]


When we choose we get the (local) Green’s function of the magnetic subsystem and the system of equations is closed. The self-consistency cycle111We did not show the calculation of the expectation values and the chemical potential for readability. The expectation values have to be calculated with the projected functions , and while the chemical potential is determined by the full Green’s function . now reads

where the self-energy determination and the CPA formalism are strongly correlated.

4 Free energy

In the previous sections we determined the Green’s function and the internal energy, but only for a given magnetization . To decide which magnetization the system actually favors we want to calculate the free energy and find its minimum, according to . To abbreviate the notation and avoid confusion with the entropy we will use for the local moment magnetization in this section. We note that is not the total magnetization of the full system of local moments and electrons. But due to the self-consistent determination of described in Sec. 3, is a unique function of . Thus we can see the local moment’s magnetization as the order parameter of the whole system.
The free energy is given by its general formula


Note that the magnetization is considered as a fixed (order-) parameter, i.e. an independent thermodynamic variable. Using the product rule and subtracting on each side we get


Integration of this equation with the condition




Since we know the internal energy from the previous sections we can calculate the free energy if we have access to the entropy at .
Equation (26) allows us to calculate the full temperature dependence of the free energy for a special magnetization. When we calculate it for many values of we get an ensemble of functions from which we can get the magnetization dependence at a special temperature, . If we find its minimum we get the magnetization at the temperature :


Since this formula is exact, the quality of the results depend only on the accuracies of the internal energy and the entropy .

4.1 Zero temperature entropy in the concentrated lattice

We cannot determine the entropy in general so we make some approximations to find an expression for . The zero temperature entropy is defined as


where is the number of ground states according to the magnetization . First we assume that total number of states is given by the product of the number of states of the local moment and the itinerant electron system222This means that the number of states of one subsystem is independent of a special state of the other., . This is plausible due to the different orders of magnitude of the dynamics of the local moments and the itinerant electrons. Thus the total entropy is the sum of the single entropies


The assumption of separable electron/spin states is an ansatz which would be questionable, e.g., in systems where electrons are bound to distinct spins. For those cases other, more complex, methods to compute the entropy have to be found.
Let us start with the entropy of the local moments. Again due to the higher electron dynamics the local moments see no single static electron. Thus we can approximate the action of the electrons on the local moments as an effective field which is equal for all lattice sites. This is a similar situation to the ideal paramagnet except that the field depends on electronic properties and the magnetization itself. We do not have to calculate directly, but we can say that each configuration of local moments () has the same energy as long as it has the same configurational average . Just as well, configurations with different averages do have different energies. At only one energy level contributes to a thermodynamic average and therefore only states with the same configurational . So we can conclude that the thermodynamic magnetizations equals the configurational one, . Thus, for a given , we have to count all possible configurations that have the same configurational average to get the zero temperature entropy. The identity of configurational and thermodynamical average is of course not true for , but in this case we do not need it, because we determine the thermodynamical average by the minimization of the free energy. For we can give an analytical expression of the entropy


and for we have to count numerically.
The itinerant electrons see more or less a static potential of the local moments. That is why we use the expression of the Fermi gas


to evaluate the zero-temperature entropy. Note that the mean values are calculated by the full theory of section 3!

4.2 Zero temperature entropy in the diluted lattice

We need the same simplifications as in the previous section. Therefore nothing changes in the formula for the electronic entropy (32), except that we get from the CPA Green’s function.
For the local moments we define the magnetic subsystem’s magnetization at as with . When we still assume that the local moments interact only with an effective field created by the electrons (corresponding to an ideal paramagnet or independent spins, respectively), we do not have to change the general procedure to get . Actually the entropy per lattice site stays the same as in the concentrated case. Thus we get


Note that the disorder itself leads to no (magnetization dependent) contribution to the entropy in this case, but only the dilution. Thus special disorder effects on the magnetization, e.g. found in Ref.[21], are beyond the scope of this paper. They could, e.g., play a role in materials which tend to form clusters.
It is a big advantage that we do not need to map the KLM onto a Heisenberg model to calculate the local moment’s properties, especially in the diluted system. This would involve extra disorder[10, 22, 23] within the Heisenberg model to be calculated separately from the electronic disorder already kept within the CPA formalism. Just as the general inconsistency of treating one system with two models (KLM, Heisenberg) this problem is avoided in our treatment. Since our theory is based on translational invariance within each component we do not get percolation effects. Those can be crucial at low doping if there is a short range interaction between the local moments. But even for an interaction range slightly larger than next-neighbor, the percolation threshold is strongly reduced[24]. Since the interaction between local moments in the KLM is assumed to be RKKY-like and therefore long ranged, percolation effects should play a minor role.
As mentioned before, in systems which are not translational invariant, the entropy had to be calculated more appropriate, which would be a difficult task indeed.

5 Results

Figure 1: (color online) The quasi-particle density of states of the concentrated system for various magnetizations . The QDOS splits into two subband at and . For decreasing spectral weight is transferred from upper to the lower subband or vice versa (MCDA). The mean-field QDOS (dashed lines) is only the shifted (by ) free QDOS. Which magnetization is actually present for a specific parameter set, has to be calculated by the minimization of the free energy. Parameters: , eV, eV,

Our main interest is focussed on the dependence of the Curie temperature on the significant model parameters. That’s why we first want to discuss these dependencies in the concentrated () system. After that we come to the diluted one. Finally we want to use model parameters which are suitable for the real system of GaMnAs to compare our theoretical results with those of the experiment.
It turns out that in the KLM the term in Eq. (26) is much smaller than . Thus we can neglect this in a very good approximation. Since was the only term with an explicit temperature dependence we get a simplified formula


and its inverse function . It means that the magnetization curve is only dependent on zero temperature quantities333Zero temperature does not mean the absolute ground state in our work, since we calculate for different magnetizations, which are not equal in energy. Especially we can use (34) to calculate the Curie temperature, when we set .
The lattice is assumed to be simple cubic in this model study with a next-neighbor tight-binding dispersion


where is the free bandwidth.

5.1 Concentrated System

To calculate the quantity of interest is the internal energy, in our case. Thus we should have a look on the quasi-particle density of states (QDOS) , since it has the main influence on as it can be seen in Eq. (5). In the concentrated system the QDOS splits into two subbands at different energies (cf. Fig. 1). One is situated at (lower subband for and upper for ) and the other at . In contrast to the MF approximation these subbands remain at this energy range for all values of , only the spectral weight is shifted from the upper to the lower subband for decreasing magnetization, or vice versa. This means a much lower energy difference in the MCDA than in the MF approximation. Comparing this with Eq. (34) shows that the MCDA results should give lower Curie temperatures as the MF approximation.

Figure 2: (color online) Curie temperature vs. coupling for various electron densities . In contrast to the mean-field result saturates for large or is growing slowly, respectively. At the MF approximation (dashed line, ) increases quadratically with . Parameters: , eV

Indeed this is the case, e.g. when we plot over (Fig. 2). The MF Curie temperatures are much higher444Because of the high of the MFA we usually use a smaller for MF results in this work to have a better comparison to the MCDA values. than those of the MCDA. Additionally we find that while we get saturation or only a slight change at large within the MCDA.

Figure 3: (color online) Curie temperature vs. electron density for various couplings . The Curie temperature of the MCDA vanishes at half-filling () even for large contrary to the mean-field approximation (dashed line, ). Parameters: , eV

The next important parameter is the electron density or the hole density in the conduction band. In the MFA, due to the shift of the majority spin’s QDOS by , the energy difference is always positive, also resulting in a positive for all (one can also see this direct connection in the shape of the --curve in Fig. 3 which resembles the shape of the free QDOS). Contrary to that the MCDA has always a vanishing at half-filling (cf. Fig. 3). Similar results can be found in other publications[14, 10, 25]. This is a very crucial result, contrary to a MF approximation which shows a maximum at half-filling (dashed line in Fig. 3). The reason for this behavior is that for the chemical potential is at the upper band edge of the lower subband. As Fig. 1 shows this upper band edge is shifted to lower energies for decreasing within our theory which means a reduction of the internal energy. Thus the energy difference in Eq. (34) gets negative resulting in a negative , being thus non-physical.

Figure 4: (color online) Curie temperature vs. free bandwidth for various couplings . In the strong coupling limit () increases approximately linearly with . At lower couplings the effect is inverse and an increase of leads to a reduction of . Parameters: ,

As the third parameter remains the free bandwidth . It is known[25] that in the strong coupling limit (, the subbands are split) becomes independent of (double exchange limit). In this case the Curie temperature is proportional to as can be seen in Fig. 4. But at lower an inverse effect occurs and an increase of leads to a reduction of the Curie temperature because the bands are not split any more. This is the typical RKKY behavior which is valid at low couplings.
We now can determine the optimal parameters for high Curie temperatures in the KLM. increases with the magnitude of the coupling . But for large saturation of occurs and the increase is limited. The electron (hole) density should be at quarter-filling for strong couplings or lower for a smaller . Finally the free bandwidth should be preferably large as long as system stays in the strong coupling regime ().
Indeed the findings in this section are similar to studies done with a mapping of the KLM onto an Heisenberg model[26, 27, 28, 29]. Also in these approaches, which go beyond mean-field, a saturation of with increasing and a vanishing of ferromagnetism below/at half-filling have been found. Thus both methods support each other. As stated before (Sec. 4.2) the use of the free energy has some advantages for computing the magnetization of diluted system. Of course one can get additional information from the free energy itself, like the entropy or heat capacity. It also can be useful to compare free energies of different magnetic phase to make statements about their existence at finite temperatures. This will be left for future work.

5.2 Diluted system

Figure 5: (color online) The quasi-particle density of states of the carriers for various dilutions . The correlated sub-bands around and arise from the interaction of the carries with the localized spins and have a total spectral weight of . Around a non-correlated sub-band exist resulting from the lattice sites without magnetic impurities. Note that the ferromagnetically saturated state, which is shown here, is not necessarily thermodynamically stable for all carrier densities and or couplings . Parameters: , eV, eV, , ,

The dependencies of on the model parameters in the diluted system stay approximately the same as in the concentrated one. But there are some additional effects due to the dilution.
In diluted systems the carriers are on lattice sites with or without magnetic impurities. Due to the interaction with the localized spins two distinct parts of the QDOS of the carriers arise (Fig. 5). One is located around (or , resp.) and results from the non-impurity sites (non-correlated part). The two other sub-bands are at and at the same positions as the quasi-particle sub-bands of the concentrated KLM (correlated part).555Note that Fig. 5 shows, for graphical reasons, a scenario of strong interaction and all parts of the QDOS belong to the itinerant carriers’ band (valence band). The correlated sub-bands should not be confused with the -bands of the DMS which are taken into account by the local moments in our model. The splitting in real DMS would be much smaller.. The positions of the sub-bands are not affected by the concentration , but the spectral weights are. In Fig. 5 one sees that the correlated subbands have the spectral weight and the non-correlated . This means, as long as the correlated bands are split from the non-correlated band, that we get an effective filling of the correlated band and, e.g., half-filling of the correlated bands occurs at .

Figure 6: (color online) Curie temperature vs. electron density for various dilutions . A finite positive Curie temperature only occurs below half-filling of the correlated band (). Parameters: , eV, eV,

As seen in the case of the concentrated KLM () ferromagnetism at half-filling of the sub-bands is not thermodynamically stable. Thus there are positive Curie temperatures only for (partly filled lower correlated subband, cf. Fig. 6) or (partly filled upper correlated subband) . For the chemical potential is in the non-correlated band (for at least) andthe lower/upper correlated subband is completely filled/empty resulting in a vanishing of ferromagnetism.
Secondly the maximum at quarter-filling is reduced for decreasing . It can be understood, in the strong coupling regime, with the reduction of the effective bandwidth of the correlated band[6], . Since we know that is proportional to for large the Curie temperature should be in the diluted system. Note that the strong coupling regime is now defined by the effective bandwidth, . Thus with decreasing a system can get into the strong coupling limit for constant .
One of the best known DMS is GaMnAs. To model this material we fix some parameters from now on. As seen from photoemission experiments[30] the coupling is about eV. Furthermore we approximate the bandwidth from ab-initio calculations[31] to eV. Since we use a simple cubic tight-binding dispersion we take into account only the main part of the ”ab-initio”-DOS below/around the fermi-level for this estimation. Furthermore it is useful to change to the hole picture, where we define the hole density since the bands are completely filled for .
Of course, in a real material other mechanisms besides magnetic interactions play a crucial role. For example the atomic levels of different atoms will be different in general. To take those effects into account we can change the position of the non-correlated band by choosing a specific center of gravity , which we have introduced in the model Hamiltonian (2). Depending on the value of the magnetic subbands can be split from the correlated band or can lie within it. Especially this determines which kind of holes are created by filling the band with carriers. When the upper magnetic subband lies above the non-correlated band, holes preferentially occupy magnetic sites for low doping leading to a large ”magnetic hole density” (cf. Fig. 7). This will be reversed when the magnetic subband gets to lower energies.

Figure 7: (color online) Electronic QDOS of the diluted system for two different centers of gravity of the noncorrelated band . The total QDOS (black line), the projected QDOS of the magnetic sites (red dashed line) and the Fermi level (black vertical line) are shown. Top: eV. The upper subband stemming from the magnetic sites is slightly above the noncorrelated band and the lower one is broadened within the noncorrelated band. Holes exist above the Fermi level (grey area) almost completely in the magnetic QDOS leading to a ratio (ratio for all holes ) . Bottom: eV. The upper impurities’ subband is within the noncorrelated band. The number of holes in the magnetic QDOS is reduced to . Parameters: , eV, eV, , , , K

The reduction of with increasing has two different effects on . For low carrier densities (left of maxima of the parabola-like curves in Fig. 6) a decreasing means a reduction of . On the other hand, systems with reach a finite Curie temperature not before a certain amount of holes on magnetic sites is transferred to nonmagnetic sites (cf. Fig. 8).

Figure 8: (color online) Curie temperature vs. the center of gravity of the noncorrelated band for various hole densities . As long as chemical potential is in the correlated band is large. When the correlated band (and therewith ) gets into the noncorrelated band (here at eV) decreases for low hole densities. For hole densities finite Curie temperatures occur only in the non-split regime. Parameters , eV, eV,

Figure 9 shows clearly the dependence of on the filling of the magnetic subband. As long as does not reach a critical value a finite Curie temperature exists. For the case that the correlated subband is far above the non-correlated band and a large this critical filling would be approximately one. If the subband comes near (but not into) the non-correlated band hybridization effects with the non-correlated band become larger and a small amount of spectral weight is transferred to the energy region of the non-correlated band. Thus the spectral weight of the correlated subband outside the non-correlated band decreases below . Nevertheless the complete actual filling in Fig. 9 can be connected to the kinks in the curves which are at the same position where reaches zero. These kinks disappear when the upper correlated subband gets into the non-correlated band. This means that a complete filling of the subband cannot be achieved even at hole densities , but at much higher hole densities (cf. Fig. 7). Thus the Curie temperature stays above zero for . Even though in this case ferromagnetism occurs over a broad range of the hole density, the maximum is heavily reduced. A very similar picture has been found for dynamical mean-field/Monte Carlo calculations[13].

Figure 9: (color online) Top: Curie temperatures vs. hole density for different centers of gravity . Bottom: The according hole density on the magnetic sites . is heavily affected by the filling of the magnetic subband (cf. Figs. 7, 8). When the upper correlated band is split from the non-correlated band (eV), increases rapidly with . In this case a distinct critical ratio can be found where ferromagnetism breaks down (). If the subband is within the correlated band there is ferromagnetism over a broad range of hole densities but the maximum is reduced. Parameters: , eV, eV,

In fact ab-initio calculations predict that some amount of states, arising from the doping with manganese, is slightly above the non-correlated band[31]. This is in agreement with measurements of Cho et al. [8, 9] on the behavior of ferromagnetism. They state that for low hole density an increase of leads to an increase of . Beyond a specific decreases and finally breaks down as calculated in this work in the ”split-up” regime. Unfortunately Cho et al. cannot give absolute values of . Why do experiments and ab-initio calculations show a maximum at as found by Jungwirth et al.[5] in contrast to our model theory? One reason can be that the correlated bands are partly within the non-correlated band which allows a finite even at , because the correlated band is not completely filled in this case. But more important is that the -levels of the impurities are threefold degenerated. One hole in these three states mean effectively a ”third filling” of the correlated band[32]. Thus even for the correlated band is not completely filled, but on the left side of the maxima of the parabolas in Fig. 9 with an effective filling of . This would indeed explain the increase of Curie temperatures with increasing hole density and the breakdown of ferromagnetism at large .
Since we have seen that highest Curie temperatures occur in the ”split-up” regime and ab-initio calculations also predict this scenario we choose a where the bands are split to investigate the influence of manganese doping on . In this case an only partly filled correlated band is necessary for finite s. As the real variation of the hole density with doping is not completely clear we propose three different types of fillings/compensations in Fig. 10.

Figure 10: (color online) Curie temperature vs. doping rate . Three curves are plotted for different compensation types. A constant hole density (red line, ) or compensation (black line,) leads to finite for or , respectively. When is larger than half-filling of the correlated band decreases. A relative compensation (green line, ) prefers ferromagnetism at every doping as long as is large enough (cf. Fig. 3.) Symbols are from the experiment[3]. Parameters: , eV, eV, eV

The first is a constant compensation resulting in a hole density . For there is of course no ferromagnetism possible since the ordering mechanism is carrier mediated. With increasing doping the system has the optimal where the maximum is reached (cf. Fig. 9). After that further impurities decrease the Curie temperature again. The second type of compensation shall result in a constant . Also in this case we need a finite doping to get a positive since has to be larger than . But with increasing the Curie temperature changes only slightly. Finally there could be a constant relative compensation . We have chosen in this work. Thus the hole density is for all near its optimal value and there is a large finite . Since there is the same effective filling and the system is in the strong coupling limit, the dominant parameter is the effective bandwidth . The Curie temperature scales therewith almost only with the effectice bandwidth as it is usual in the strong coupling regime (cf. maxima of in Fig. 6). This results in the curvature .
Of course these compensation mechanisms are idealized and in reality there is probably a combination of these three basic types. But it can be seen that the hole compensation is indeed a very important effect for the DMS.

6 Summary

We have performed a model calculation to describe carrier mediated magnetic ordering of local moments. To do that we used a Kondo lattice model with ferro- or antiferromagnetic coupling between the carriers and the local moments. The electronic subsystem is treated in an equation of motion method to calculate the Green’s function and the internal energy. From the internal energy we get the free energy which can be minimized according to the magnetizion of the local moments. This yields the actual magnetization of the system. To include disorder and dilution of magnetic impurities we have extended this method by a coherent potential approximation and a proper alloy analogy.
With this method we investigated the influence of several model parameters on the Curie temperature. We found that the optimal values are around quarter-filling of the conduction band in the strong coupling regime. Additionally the free bandwidth should be as large as possible as long as the strong coupling limit is fullfilled. If is too large () decreases. The effect of the bandwidth plays also a leading role in diluted systems. Since the effective bandwidth of the correlated band, which arises from the interaction of carriers and (diluted) local moments, is proportional to the square root of the doping, , increasing enhances the Curie temperature. At half-filling of the correlated band no ferromagnetic ordering exist, which shows the importance of hole compensation in diluted magnetic semiconductors. It is also necessary for high s that the correlated band is separated from the non-correlated band and that the chemical potential is within the correlated band. Finally we have compared the calculated values of with experimental ones of GaMnAs which are in good agreement to each other.
Since we calculate the free energy it is possible to determine other quantities like the entropy or heat capacity of a system. Also free energies of different (magnetic) phases could be compared to see which phase is actually present at finite temperatures. We will leave this for future work.


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