Dept. of Physics & Astronomy, LSU Center for Computation and Technology, LSU
Published
Feb. 20, 2022
Introduction
While this represents nothing particularly new about this well-studied model, I have found most references on this subject gloss over or miss certain points that I think are important for getting the full picture of this model and what it can teach us regarding topology in condensed matter systems.
The Su-Schrieffer-Heeger model, or SSH model for short, is in a sense one of the simplest models of topology and the resulting edge states (the bulk-boundary correspondence), so a full analysis of it helps to shed light on other models in higher dimension with topologies that might be a little harder to imagine.
The model is a simple tight-binding model representing polyacetelyne C2H2 but it also has an artificial particle-hole symmetry which when interpretted as a model of Bogoliubov-de-Gennes quasiparticles (in a p+ip superconductor) it becomes an exact symmetry.
Model definition
The molecular chain is a combination of weak bonds and strong bonds and thus has two (low energy) configurations that are degenerate:
Figure 1. Two configurations for polyacetylene leading to different hoppings between carbon atoms (t1 vs. t2). We can label the chain with two sublattices A and B, and we have a unit cell that includes two atoms (as indicated by the gray square).
The tight-binding model for the SSH model takes the form
where n labels the unit cell A and B are the different sublattices with hoppings t_1 and t_2 between them.
We can introduce Pauli matrices via the sublattice space \lvert A \rangle \langle B \rvert = \sigma^+ = \sigma_x + i \sigma_y (and \sigma^- = (\sigma^+)^\dagger), giving the Hamiltonian the form
to diagonalize the model we note that \lvert{n+1}\rangle = e^{-i \hat k} \lvert{n} \rangle where e^{-i\hat k} is the translation operator by a unit cell. Using completeness \sum_n \lvert n \rangle \langle n \rvert = 1 we can write down our Hamiltonian as
This gives us a Brillouin zone as well with k\in[-\pi,\pi). Here we write the k-space Hamiltonian out in three ways for pedagogical reasons
and finally the general form
where for our model \epsilon_0(k) = 0, d_x(k) = t_1 + t_2 \cos k, d_y(k) = t_2 \sin k, and d_z(k) = 0. If we write \mathbf d(k) = d(k) ( \cos \phi_k \sin \theta_k, \sin \phi_k \sin \theta_k, \cos \theta_k), then the general solution to this two-level problem is
with solution for the lowest band (\epsilon_-(k))
The nice thing about these \lvert u_k \rangle is they are easily represented by points on the Bloch sphere.
For our model , we have \theta_k = \pi/2, and e^{i\phi_k} = (t_1 + t_2 e^{-i k})/|t_1 + t_2 e^{-ik}|.
Note that only the unit vector
controls the wave function (and as we’ll see, the topology).
Lastly, the energy bands look like
Figure 2. The energy bands of the SSH model with t2 = 0.75t1.
Berry connection, Berry phase, and polarization
For the necessary mathematical machinery, we refer to Ch. 3 of . The Berry connection is then given by
We can compute the Berry phase for this band which is exactly related to the polarization (see Ch. 4 of )
It is tempting to change variables in the integral to \oint d \phi_k, but we need to understand what the closed curve \oint represents. Since d_z=0 we can think purely in terms of the equator of the Bloch sphere and either \phi_k makes it around the sphere or it does not as indicated in Fig. 3 below.
Figure 3. The two situations for this model: either \phi_k wraps around the origin or not. (red) t_1<t_2 we call "topological" and the Berry phase indicates a winding number of 1. (gray) t_1>t_2 has no winding number and is labeled "trivial".
From this information, we can read off what the results from the Berry phase calculation for polarization becomes
The first case t_1 < t_2 is represented in red in Fig. 3 and we call it “topological” while the case t_1 > t_2 we call “trivial”.
One might wonder at this point why these two phases are distinguishable at all since Fig. 1 shows two configurations that when rotated about an A site appear to be exchanged. The answer to this comes from two sources (1) domain walls between configurations (to be explored in a future post) and (2) edges. Fig. 1 shows the situation with edges: either the lattice ends with a strong bond or a weak bond. Both of these situations come into full focus when we consider edge states resulting from the topology.
Symmetries
Aside from translation symmetry, which we have already used to find H_k, what other symmetries are in the problem? In particular, what discrete symmetries can we identify? The model as written down in has the following symmetries:
Time reversal symmetry
Chiral symmetry
Particle-hole symmetry
Inversion symmetry
Each of these is important for the topology of the problem.
Time-reversal symmetry
The first symmetry we identify is the anti-unitary symmetry of time-reversal. In this model it takes the form T = K where K is complex conjugation (in the real space basis).
In terms of our k-space Hamiltonian we have
For a the general two-band Hamiltonian , we have
In general, this does not constrain our problem enough to give us topology since if we imagine taking k and mapping it onto the sphere (some closed path) given the above constraints, at k=0 and k=\pi\mathbf d is constrained to be in the xz-plane.
Under these constraints, any path can be continuously deformed onto just a single \mathbf d(k) \equiv \mathbf d_0, indicating a trivial topology.
We clearly need something to limit our available paths.
Chiral Symmetry
Chiral symmetry is an odd symmetry. It is unitary, however the symmetry relates the positive and negative energies. In particular, the chiral operator \sigma_zanti-commutes with the Hamiltonian \{H, \sigma_z\} = 0 or in terms of its action on H_k
We can directly discern from this that for every positive energy states we can construct a negative state \sigma_z \lvert E_k \rangle = \lvert - E_k \rangle. For the two-level problem we are working with, the core issue constraint is
This constrains us to be on the equator (see Fig. 4)
Figure 4. The constrained space from chiral symmetry is just the equator of the Bloch sphere, and the resulting topological number is just the winding number about the origin (how many times you go around the equator).
The winding number can be defined safely with the gauge chosen in , this is the polarization but now with \mod e, so to differentiate it we call it
However, we would like a gauge-independent quantity and if we let \lvert u_k \rangle \rightarrow e^{i\alpha_k} \lvert u_k \rangle then we can change the above expression by an even integer.
To remedy this, we first note that general solutions now take the form
And we can in fact obtain the phase difference \phi_k by a slight modification of the Berry connection to include the chiral operator
Thus chiral symmetry gives us a strong constraint which leads to an integer topological number \mathbb Z.
This winding number can also be computed directly from the Hamiltonian. Two natural ways of getting it include use of the \mathbf d(k) vector
and the second, which generalizes to multiple bands requires us put our Hamiltonian in the form
and for the matrix h(k) we have
Physically, this symmetry relies on there not being a term proportional to \mathbb{I} or \sigma_z in the Hamiltonian which in terms of sublattices means that no potential is allowed and we are only allowed hoppings from the A sublattice to the B sublattice.
In polyacetyline this is not an actual symmetry since no physical process prevents hopping from within a sublattice. We therefore need to argue for some other symmetry in the problem that leads to topology.
Inversion symmetry
The inversion symmetry in the SSH model (equivalently, reflection symmetry or 180-degree rotation symmetry) is best understood by taking Fig. 1 and flattening it out as in Fig. 5 below
Figure 5. The inversion center (gray vertical line) takes the A sublattice to the B sublattice as well as exchanges the unit cells n and -n.
This is a traditional unitary symmetry of the problem and its action on the k-space Hamiltonian is to relate k to -k and to exchange the A sublattice with the B (this is accomplished with \sigma_x)
In terms of the two-band system
Our first hint of two topologically distinct classes comes from there being two inversion symmetric polarizations possible P = 0 \mod e or P = e/2 \mod e since in both cases P = -P \mod e (polarization changes signs under inversion).
Now the unit vector \hat{\mathbf d}: S^1 \rightarrow S^2 maps a closed path onto the (Bloch) sphere. If we permit any continous change in \hat{\mathbf d} every closed path can be reduced to a single point (this is why without symmetries in 1D the topology is trivial). With the added constraint of inversion though, we have two special points \mathbf d(0) = d_x(0) \hat{\mathbf x} and \mathbf d(\pi) = d_x(\pi) \hat{\mathbf x} and the path k\in[0,\pi] completely determines the path k\in[-\pi,0). This leads to two classes of paths, one in which \mathrm{sgn}(d_x(0)d_x(\pi)) > 0 and the other in which \mathrm{sgn}(d_x(0)d_x(\pi)) < 0, and continuously changing \hat{\mathbf d} while respecting inversion symmetry cannot take one class of paths to the next. These two types of paths are represented below in Fig. 6.
Figure 6. (left) The trivial path where \mathbf d(0) and \mathbf d(\pi) are both in the positive x-direction. The solid line represents the path for k\in[0,\pi) while the dashed line represents k \in [-\pi,0). The green area (inclosed by the dashed lines) is exactly the same as the red area but oppositely oriented and thereby they cancel each other by Stokes' theorem when one calculates P = \frac{e}{2\pi} \oint dk A(k) = 0 \mod e. (right) The topological path where again the path k\in[0,\pi) is represented by a solid line while the dashed line represents k \in [-\pi,0). In this case, the way k relates to -k guarantees that upon going over the whole Brillouin zone, Stokes' theorem will map out half of the area of the sphere modulo an integer times the full area or in other words P = \frac{e}{2\pi}\oint dk A(k) = e/2 \mod e.
This suggests a simple way to differentiate topological and trivial phases known as symmetry indicators.
If we look at the inversion symmetric points, the Hamiltonian has the form
The inversion operator at these points is simply \sigma_x with \lvert{u_{k=0}}\rangle and \lvert{u_{k=\pi}}\rangle both eigenvectors of that operator with eigenvalues \xi_{0} = \mathrm{sgn}(d_x(k=0)) and \xi_\pi = \mathrm{sgn}(d_x(k=0)), respectively.
There is then a \mathbb Z_2 index which we can define simply by
(we have defined \tilde \nu_{\mathbb Z_2} = (-1)^{\nu_{\mathbb Z_2}}.) The \mathbb Z_2 invariant is also computed, as we have suggested, by the polarization
such that P = \frac{e}{2}\nu_{\mathbb Z_2}.
By just looking at two points in the Brillouin zone, we can discern if the phase is topologically nontrivial. In summary, inversion symmetry alone gives us \mathbb Z_2 topology.
Particle-hole symmetry
The last symmetry we consider is actually a combination of previous symmetries, particle-hole symmetry for this problem will be the anti-unitary symmetry made by combining time-reversal symmetry and chiral symmetry. In fact, for this problem
It acts on our k-space Hamiltonian such that
In terms of the two-band model we have the constraints
These constraints are suprisingly close to the constraints place upon us due to inversion symmetry except for \epsilon_0(k) which here must be odd in k instead of even in k.
However, that detail does not affect the wavefunctions which only follow \mathbf d(k) and so by very similar logic to inversion symmetry if we have this particle-hole symmetry, we have a \mathbb Z_2 topology.
Cartan Classification
Each individual Hamiltonian such as has their own particular symmetries. However, to speak of topology one must think closely about what terms could be added to the Hamiltonian.
This is seen very clearly in the SSH model where we have enumerated many symmetries, but have argued that some of them (such as the chiral symmetry) do not make sense for the physical symmetry.
Nonetheless, it is a useful exercise to take each symmetry seriously and build out what topology it implies.
For the two-band systems suggested by the SSH model we have done just that, and the result matches what is known from topological classification .
T
C
S
Topology
0
0
0
0
1
0
0
0
0
1
0
\mathbb Z_2
0
0
1
\mathbb Z
1
1
1
\mathbb Z
T represents time reversal, C represents particle-hole symmetry, and S represents chiral symmetry (0 is no symmetry, 1 is that it is present).
Additionally, we can include inversion symmetry. The only relevant combination is time-reversal and inversion, which leads directly to d_z(k) = 0 and allows us to use the arguments for chiral symmetry to obtain a \mathbb Z invariant (though with a finite \epsilon_0(k) which needs to be considered only for purposes of having a direct gap between bands as well as when taking into account Fermi energies)
T
Inversion
Topology
0
1
\mathbb Z_2
1
1
\mathbb Z
All of this applies to the entire lower band of this system, when we are in the insulating state. Partially filled bands don’t allow us to perform many of the full integrals over the whole Brillouin zone and therefore cannot be classified as we have mentioned.
Conclusions
This post has been mainly concerned with the bulk classification of the topology inherent in the SSH model, carefully going through each symmetry and its relation to the topological classification (as well the corresponding topological numbers).
In this system, the main observable for the model are edge states, which we have not discussed here.
Footnotes
References
Berry Phases in Electronic Structure Theory Vanderbilt, D., 2018. Cambridge University Press.
Periodic Table for Topological Insulators and Superconductors Kitaev, A., 2009. AIP Conference Proceedings, Vol 1134(1), pp. 22--30. American Institute of Physics. DOI: 10.1063/1.3149495
Topological Insulators and Superconductors: Tenfold Way and Dimensional Hierarchy Ryu, S., Schnyder, A.P., Furusaki, A. and Ludwig, A.W.W., 2010. New Journal of Physics, Vol 12(6), pp. 065010. IOP Publishing. DOI: 10.1088/1367-2630/12/6/065010