Research Article | Open Access
Shosuke Sasaki, "Spin Polarization Curve of Fractional Quantum Hall States with Filling Factor Smaller than 2", International Scholarly Research Notices, vol. 2013, Article ID 489519, 19 pages, 2013. https://doi.org/10.1155/2013/489519
Spin Polarization Curve of Fractional Quantum Hall States with Filling Factor Smaller than 2
Kukushkin et al. have measured the electron spin polarization versus magnetic field in the fractional quantum Hall states. The polarization curves show wide plateaus and small shoulders. The 2D electron system is described by the total Hamiltonian (). Therein, is the sum of the Landau energies and classical Coulomb energies. is the residual interaction yielding Coulomb transitions. It is proven for any filling factor that the most uniform electron configuration in the Landau states is only one. The configuration has the minimum energy of . When the magnetic field is weak, some electrons have up-spins and the others down-spins. Then, there are many spin arrangements. These spin arrangements give the degenerate ground states of . We consider the partial Hamiltonian only between the ground states. The partial Hamiltonian yields the Peierls instability and is diagonalized exactly. The sum of the classical Coulomb and spin exchange energies has minimum for an interval modulation between Landau orbitals. Using the solution with the minimum energy, the spin polarization is calculated which reproduces the wide plateaus and small shoulders. The theoretical result is in good agreement with the experimental data.
In this paper, we examine the electron spin polarization in the FQH states with the filling factor . Before the examination, we see here the investigations on the FQHE briefly.
The fractional quantum Hall effect was discovered by Pan et al. [1, 2]. The quasi particle with a fractional charge and its wave function were introduced by Laughlin using the variational method [3, 4]. Many physicists developed it [5–7]. Jain proposed the composite fermion theory [8, 9]. Thereafter, the FQH states with the nonstandard filling factors have been investigated by employing various methods as in the references [10–14]. These theories assume the various types of the quasi particles and their mixing. On the other hand, Tao and Thouless [15, 16] examined the case that the lowest Landau levels are partially filled with electrons. Their method is very important to investigate the FQH states. We have developed the Tao-Thouless theory and have found the most uniform configuration of electrons. It has been proven that the configuration is unique for any filling factor . The configuration minimizes the expectation value of the total Hamiltonian.
The Coulomb transitions conserve the component of the total momentum where the -direction indicates the current direction. The conservation law produces energy gaps for the specific filling factors. For the other filling factors, we have found the gapless structure and peak structure [17–23]. The theory can well explain the behaviors of the FQHE at without any quasi particles.
On the other hand, the electrons in FQH states with occupy the higher Landau levels. Therein, many experimental and theoretical investigations [24–43] are carried out and various interesting phenomena are discovered. Also, the electron spin polarization is investigated for the FQH states with by the papers [44–49].
Although the function form of the spin-polarization versus magnetic field is very important for investigating the FQHE, there is no theoretical calculation of the function shape quantitatively. In this paper, we calculate the spin-polarization versus magnetic field at by developing the previous method in the references [17–23].
Kukushkin et al. have measured the electron spin-polarization versus magnetic field . They clarified the function forms at twelve filling factors in . Although their experiments are rather old data, the obtained function forms give us the important knowledge.
Their results are shown in Figure 1. Hereafter, we describe the electron spin polarization by the symbol . Then, means a fully polarized state. The experimental polarization curves have the following properties.(1)The wide plateau appears at for and 2/5. The wide plateau appears at for and 3/7. The two wide plateaus appear at and 1/2 for and 4/9. (2)The small shoulder appears at for and 2/5. The small shoulder appears at for and 3/7. The two small shoulder appear at and 3/4 for and 4/9.
As shown in Figure 1, the polarization curve resembles the curve. The polarization curve resembles the curve. Also, the curve resembles the curve. The characters mentioned above indicate that the shape of the spin polarization curves depends mainly upon the numerator of the filling factor. The numerator means the electron number per unit configuration (see ). Therefore the polarization belongs to electrons (not holes). In this paper we clarify the origin of the polarization curve.
We shortly describe the fundamental properties of the quasi-two-dimensional electron system below. We illustrate a quantum Hall device where the directions of the axes , , and are taken, as in Figure 2. Then, the vector potential, , has the components: where is the strength of the magnetic field.
The Hamiltonian, , of a single electron in the absence of the Coulomb interaction between electrons is given by where and indicate the potentials confining electrons to an ultrathin conducting layer in Figure 2. Therein is an effective mass of electron, and is the electron momentum. The effective mass differs from material to material and the value in GaAs is about 0.067 times the free electron mass. The eigenvalue problem of this Hamiltonian is solved and the single electron wave function is expressed as follows: where is given by
Therein, is the wave function of the ground state along the -direction, is the Hermite polynomial of th degree and is the normalization constant. We call the Landau level number. Also, the eigenenergy is given by where is the ground state energy along the -direction is the potential energy in the -direction.
When there are many electrons, the total Hamiltonian is given by where is the total number of electrons and is the single particle Hamiltonian of the th electron without the Coulomb interaction as
The many-electron state is characterized by a set of Landau level numbers and a set of momenta . The complete set is composed of the Slater determinant as
This state is the eigenstate of . The expectation value of the total Hamiltonian is denoted as which is given by where is the expectation value of the Coulomb interaction defined by
Hereafter, we call “classical Coulomb energy.” We divide the total Hamiltonian into two parts , and , as follows: where is constructed only by the off-diagonal elements and depends upon only the relative coordinate. Therefore, the total momentum of the -direction conserves in this system. That is to say, the sum of the initial momenta and is equal to the sum of the final momenta and via Coulomb transition as follows:
At a filling factor smaller than 1, the ground state of satisfies the following properties.(1) electrons exist in the lowest Landau levels with . (2)The electrons most uniformly occupy the lowest Landau levels. Then, the classical Coulomb energy takes the lowest one. The electron momenta are related to each centre position as in (4).
For any filling factor, we can find only one electron configuration in Landau states which is the most uniform and has the minimum energy of . The proof is done in . When the magnetic field is weak, there are many spin arrangements for a given configuration. These spin arrangements construct the degenerate ground states of . The interaction Hamiltonian yields the quantum transitions among the ground states. We examine the interaction in the next section.
2. Coulomb Interaction between Up- and Down-Spin States (Equivalency between Coulomb Transition and Spin Exchange Interaction)
The degenerate ground states have the same momentum set corresponding to the most uniform electron configuration. The Hamiltonian given by (11) acts between two electrons. We indicate the spin states by and for up- and down-spins, respectively. Then, all the initial spin states with the momentum pair , are described as
When these states transfer via , their final states are described as follows: where and indicate the final momenta via the Coulomb interaction. We consider the transitions only between the degenerate ground states. Therefore, the final momentum set should have the minimum energy of . Accordingly, the final momentum set is equivalent to the initial momentum set because of the uniqueness of the electron configuration for the ground state of :
The case of is removed because the diagonal matrix elements of are zero. Applying (15), the final state becomes which is the same as its initial state. Also becomes . In the two cases, the final state is identical to the initial state, and therefore the matrix elements of are zero. Accordingly, nonzero matrix elements are
We examine the following three cases.
Case 1. Consider
Case 2. Consider
Case 3. Consider
The Coulomb transition in Case 1 is shown in Figure 3. The open circle indicates the up-spin state and the filled one the down-spin state. We describe the momenta after the transition by the symbols and which are given by
This Coulomb transition is equivalent to the following process: The spin at site 1 flips from up to down and the spin at site 2 flips from down to up simultaneously without changing the momenta. Thus, the Coulomb transition of Case 1 is equivalent to a spin exchange process which is described by the interaction . Therein, is the spin transformation operator from down- to up-spin state and is the adjoint operator of . There is another Coulomb transition given by (16b) which is equivalent to . Accordingly, the Coulomb transition between the two electrons at sites 1 and 2 is expressed as where was already defined by (18a). In this Coulomb transition, the classical Coulomb energy in the initial state is exactly equal to the one in the final state.
The momenta after the transition are described by the symbols , , the values of which are given by
The Coulomb interaction of Case 2 is equivalent to the following spin exchange interaction between an electron pair placed in second nearest-neighboring orbital pair: where is the coupling constant defined by (18b).
We show the most uniform configuration of electrons for the two cases of and in Figures 6(a) and 6(b), respectively, where the spin-states are numbered sequentially from left to right, as indicated by the green color.
In the state, the nearest electron pairs have the coupling constant and the second nearest electron pairs have the coupling constant . At , the nearest electron pair is placed in the second neighboring orbital pair, and so the coupling constant is . The second nearest electron pair is placed in the third neighboring orbital pair and so the coupling constant is as shown in Figure 6(b). Thus, it is noteworthy that the site number (namely, electron number) is different from the orbital number.
In the third or further nearest electron pair, another electron is inserted as in Figures 6(a) and 6(b). Therefore the interaction between the third nearest electrons is quite weak due to the screening effect of the interposing electron, and so may be neglected.
At the most effective interaction is obtained as follows: where the operator indicates the transformation from a down- to up-spin state of the electron at the th site. This Hamiltonian, (25), yields the quantum transition between the degenerate ground states. When the external magnetic field is applied in the -direction, the Hamiltonian becomes where is the effective -factor, is the magnetic field, is the electron spin operator in the -direction, and is the Bohr magneton. The matrices (the Pauli spin matrices) are explicitly indicated below:
We can obtain the Hamiltonian for other filling factors. The Hamiltonian for and is given, respectively by;
3. Isomorphic Mapping from the FQH State to One-Dimensional Fermion State
We examine the following mapping from a single spin state to a fermion state. The down-spin state is mapped to the vacuum state , and the up-spin state is mapped to the one fermion state , where is the creation operator
Then the spin operators , , and are mapped to the operators of the fermion system as
Next, we find the isomorphic mapping from many-spin states to many-fermion states. Two examples of the mapping are written as follows:
It is noteworthy that the multiplying order of creation operators is the same as the order of the up-spins. The operators and satisfy the anticommutation relations as follows:
The products of the spin operators , , and are mapped to the products of fermion operators as follows:
We exactly solve the eigenvalue problem of this Hamiltonian.
New operators and are introduced as follows: where is the cell number. Then the Hamiltonian (34) becomes where is the total number of cells given by for the total number of electrons . We apply a Fourier transformation given by (38) to the operators , , , and and obtain and , .
In the summation in (37), the single term with a value of is expressed by the following matrix:
This matrix has two eigenvalues and which are given by
Using new annihilation operators and
the Hamiltonian (37) is expressed as follows:
Thus, we have succeeded in diagonalizing the Hamiltonian (26).
4. Magnetic Field Dependence of the Spin Polarization
The electron spin polarization depends upon the temperature. We calculate its thermodynamic mean value as follows: where is the thermal average and the minus sign comes from the negative charge of an electron. In deriving (43), we have utilized (33c), (35), (38), (41a), and (41b). The diagonal form, (42), indicates that all the eigenenergy states are expressed by the direct product of the creation operators . Therefore, the eigenstate is identified by the eigenvalue of the fermion number operator . Equation (42) shows that the eigenenergy for is and the eigenenergy for is zero. Then, the Boltzmann factor is for and for , where is the Boltzmann constant and is the temperature. Accordingly, the probability for is given by and the probability for is given by . These probabilities yield the thermal average of as which gives
Since the total number of electrons is a macroscopic value, we can replace the summation by integration as
Thus, the electron-spin polarization at the filling factor of 2/3 is expressed by (47).
First, we study the low field behavior of the spin polarization.
Equation (40a) indicates that is restricted to the following region:
Also, is in the region:
When the magnetic field takes a value between 0 and , is negative and is positive for any value of :
Therefore, is nearly equal to and is nearly equal to 1 at very low temperatures (). Then, the spin polarization is almost zero because the summation in the right hand side of (47) is nearly equal to zero. When the magnetic field increases beyond the value , the spin polarization increases continuously until it reaches the maximum value of 1. This behavior is in agreement with the experimental data in Figure 1.
When the quality of a quantum Hall device is bad, many random potentials are produced by the impurities and lattice defects. Then, the plateau in the Hall resistance curve is rounded at both ends. Also, the wide plateau in the polarization curve is rounded by the random potentials. The effect resembles that of the thermal vibration. Therefore, we include the random potential effect into the value of .
The spin polarization is evaluated by integrating the right hand side of (47). The integration has been done by using a computer program. The result is shown in Figure 7 for the parameter and . Experimental data  are plotted by red dots in the figure. We find that the theoretical result reproduces the experimental data without the small shoulder.
5. Modulation of the Intervals between Landau Orbitals
If we observe carefully the experimental spin polarization curves, namely, Figure 1, we find small shoulders in it. The structure has not been considered in the previous sections. We examine the origin of the small shoulders in this section.
Peierls studied an electron system in a one-dimensional crystal and considered the lattice distortion with the period doubling the unit cell. This lattice distortion produces new band gaps and the energy becomes lower than that without the distortion. This effect is called spin Peierls effect .
In the present theory, the spin polarization of FQH states is derived from the Hamiltonians (26), (28), and so on. If we consider a new modulation of the intervals between the nearest Landau orbitals with the period doubling the unit configuration, the spin chain Hamiltonian of FQH system resembles the one with the spin Peierls effect.
As an example, for we change the distance between nearest orbitals in the first unit-configuration longer, the one in the second unit-configuration shorter, and so on. Then, we have the four kinds of the coupling constants , , , and as shown in Figure 8.
The value of is larger than that of because the distance for the interaction path is shorter than that for . Also, holds. This distortion with the double period of the unit-configuration produces additional energies via the classical Coulomb and spin exchange interactions. We call it “interval modulation.” We calculate the total energy of this system.
We express the distance between the nearest orbitals by the symbol for nondistortion case. We consider the distortion that one of the distances between the nearest Landau orbitals becomes for an odd cell number and the other one becomes for an even cell number. Then, the classical Coulomb energy increases. The increasing value per electron is proportional to as where is the constant parameter.
Next, we examine -dependence of the coupling constants and . When , the coupling constant is weaker than because the interaction path is longer than that of . When the other case , is stronger than because the interaction path becomes shorter than that of . Therefore, there is a linear term of in and as follows: where is the coupling constant in the non-distortion case and is the proportionality constant. In order to simplify (50) and (51), we define a new dimensionless quantity as
Then the coupling constants and are expressed as
The increasing value of the classical Coulomb energy is also expressed by this dimensionless parameter as follows: where is the dimensionless coefficient as
6. Total Energy due to the Interval Modulation
Now we calculate the spin exchange energy. Using the coupling constants in Figure 8, the spin exchange Hamiltonian for is given by
Using the cell number , we introduce new operators , , , and as follows:
For one value of , (59) is expressed by the following matrix :
The four eigenvalues of are denoted by the symbols , , , and which are given by
Therein, we have assumed because the interval modulation is expected to give almost the same effect to the coupling constants and . Then, ratios between the coupling constants are expressed as follows:
Equation (53) derives the following relation:
We show the two eigenvalues and by red and black curves for , blue curves for and green curves for in Figure 9.
The difference is minimal at as seen in Figure 9. When is equal to 1, namely, nondistorted case, the energy gap disappears. Equation (61) gives the difference between and at as where we have used (53). Thus, the difference is proportional to .
The eigenenergies (61) give the diagonal form of the Hamiltonian as follows:
We calculate the thermal average of this Hamiltonian. The thermal average has been already examined in (44) which gives
Then the thermal average of the spin exchange energy is
Since the total number of electrons is a macroscopic value, we can replace the summation by integration as
We numerically calculate the integration in (67a). The dashed red curve in Figure 10 shows the calculated result of the spin exchange energy for . The dashed black curve shows the classical Coulomb energy for the parameter (see (54a), (54b)). Their sum is the total energy which is expressed by the blue curve. Then, the total energy has a minimum at a nonzero as shown in Figure 10. Consequently, the interval modulation actually occurs.
Further calculations are carried out for various values of the magnetic field in the case of . The results are shown in Figure 11. The interval modulation occurs in the region of .
We calculate the total energy for another case . The coupling constants are illustrated in Figure 12.
These coupling constants in Figure 12 produce the Hamiltonian which is described by the following matrix:
This matrix has the six eigenvalues , , , , , and , the -dependences of which are shown in Figure 13.
Figure 13 indicates the energy gap between and at . Then the interval modulation with the double period of the unit-configuration produces additional energies for the classical-Coulomb and spin-exchange interactions, respectively, as follows:
The sum of and is numerically calculated and the result is shown in Figure 14.
Therein, we have used the parameter which is the same as in the case of . This value of affects the shape of the polarization curve near the small shoulder as will be discussed in the next section. We have shown the dependence of the total energy upon for two examples. Therein, the total energy has a minimum at a nonzero in some region, of the magnetic field. The nonzero yields the stable state with the distortion (interval modulation). This mathematical mechanism is the one resembling the spin Peierls effect.
7. Spin Polarization in the Case with the Interval Modulation
We calculate the spin-polarization for the Hamiltonian (64) of . is obtained by the integration as where the four eigen-values , , , and are given in (61). We numerically calculate the spin-polarization by the following two methods, namely, easy method A and precise method B. Method A is the rough calculation under the fixed value of the distortion parameter . This method has been studied in the previous papers [53, 54] where the ratio is treated to be a constant value as in (62c). Method B is newly performed in this paper.
Method A. We use the fixed value . The other parameters are adopted to be and . Then, a small energy gap appears between and . We numerically calculate the integration in (70) by using the Mathematica program and draw the graph of spin-polarization versus magnetic field. A small shoulder appears in the theoretical curve of the electron spin-polarization as seen in Figure 15.
This curve is slightly different from the experimental data near the sharp corners and . So we choose the different value as in order to make the curvature small in the corners and . Then the small shoulder disappears. In order to maintain the small shoulder, we take a larger value . The calculated curve is shown in Figure 16. The result is also different from the experimental data. Accordingly, method A has some difficulty in explaining the experimental data. This inadequacy is improved by using the precise method B.
Method B. We carry out more precise method B where we calculate the -dependence of the total energy per electron. We find the minimum point of the total energy for various values of the magnetic field. Some examples have been already shown in Figures 11 and 14. Therein, we obtain the -value of the minimum point. The -value gives from (62c). We numerically calculate the spin-polarization by using the magnetic field dependence of the minimum point. The theoretical curve is shown in Figure 17.
Therein, we have used the parameter values , and . Thus, the calculated result is in good agreement with the experimental data. The reason is simply discussed below.
The magnetic field is sufficiently strong near the corner in Figure 15. In this region, almost all the spins have a down direction. Then the number of up- and down-spin pairs decreases and the spin exchange energy becomes small. So the increment of the total energy (67b) is nearly equal to that of the classical Coulomb energy. Then, the energy minimum appears at , namely, non-distortion (noninterval modulation). Thus, the distortion appears only near the small shoulder as in Figure 11. Due to this situation, the theoretical curve via method B is in good agreement with the experimental data.
It is examined how the shape of the polarization curve depends on the parameter . We calculate the polarization curve for the following two cases: and 0.65 in Figure 18. These calculations make it clear that the shape of the curve varies only in the neighborhood of the small shoulder when changing the parameter .
We study the case of . The spin-polarization for is given by where the eigen-energies for are numerically obtained from the matrix (68). The two calculated curves via methods A and B are shown in Figure 19. In the method B we have applied , same as in . As seen in the right panel of Figure 19, the theoretical result via method B is in good agreement with the experimental data.
We next examine the case of . The most uniform electron configuration is illustrated in Figure 20.
The electron configuration yields the Hamiltonian described by the following matrix (72):
The spin polarization is given by
Therein, the eight values for