Zhenghe's Blog

February 21, 2011

Notes 7: Examples (I)-Periodic Potentials

Filed under: Schrodinger Cocycles — Zhenghe @ 7:23 pm
Tags: , ,

From now on, I will mainly focus on the Schrodinger cocyles case.

Example 1: Constant Potentials

Let’s start with the simplest example: potential over fixed point. Equivalently, we consider constant SL(2,\mathbb R)– matrix A.

Since eigenvalues are invariant under conjugacy, we can up to a conjugacy assume A is one of  the following

\begin{pmatrix}\lambda&0\\ 0&\lambda^{-1}\end{pmatrix}, \begin{pmatrix}1&a\\ 0&1\end{pmatrix}, \begin{pmatrix}\cos2\pi\theta&-\sin2\pi\theta\\\sin2\pi\theta&\cos2\pi\theta\end{pmatrix}.

Under mobius transformation, they have invariant directions in \mathbb C\mathbb P^1 as \infty,\infty,i. Recall in Notes 3 we define functon

\tau(A,m) such that A\binom{m}{1}=\tau(A,m)\binom{A\cdot m}{1}.

In particular if u is the unstable invariant direction of A, then \ln\tau(A,u)=L(A)+i2\pi\rho(A). As the above cases, u can be \infty. But \tau(A,u) (eigenvalue) is invariant under conjugacy. Thus we can always move the computation to unit disk to avoid \infty. For simplicity let’s always denote it as \tau(A,u). Then for above matrices, we get

L(A)+i2\pi\rho(A)=\ln\tau(A,u)=\ln\lambda, 0, i2\pi\theta (note for each fixed A, \rho(A) is well-defined but not uniquely determined).

Consider A^{(E)}=\begin{pmatrix}E&-1\\1&0\end{pmatrix} and the function \rho:\mathbb R\rightarrow\mathbb R, E\rightarrow\rho(E). Let’s use Q=\frac{-1}{1+i}\begin{pmatrix}1&-i\\1&i\end{pmatrix} to move to unit disk \mathbb D. Then \mathbb R becomes the unit circle \mathbb S. Let’s consider the function N(E) (see notes 3) instead of \rho(E). It’s easy to see that for nonelliptic matrices, N is integer valued. By monotonicity of Notes 3, N:\mathbb S\rightarrow\mathbb R is not well-defined. But it’s well-defined as N:\mathbb S\rightarrow\mathbb R/\mathbb Z.  By the proof of Lemma 2 of Notes 3, we know when E changes from -\infty to \infty, so is some \cot(\theta(E))=A^{(E)}\cdot y.  Thus the change of correponding angle of the point in \mathbb S is exactly 2\pi. This implies that \deg N=1. WLOG, we can set N(-\infty)=-1, N(\infty)=0. Thus \rho(-\infty)=\frac{1}{2}, \rho(\infty)=0.

The above argument can be applied to any A^{(E-v)}=\begin{pmatrix}E-v&-1\\1&0\end{pmatrix},v\in R. Combining the equivalent description of spectrum in Notes 2 give the following description of the corresponding operator:

– the spectrum \Sigma is [v-2,v+2];
\rho|_{(-\infty,v-2]}=\frac{1}{2},  \rho|_{[v+2,\infty)}=0;
\rho is analytic and strictly decreasing in the interior of the spectrum (v-2, v+2).

Example 2: Periodic Potentials

Next let’s consider periodic potential case. Namely, (X,f,\mu)=(\mathbb Z/(q\mathbb Z), f, \mu), where f: \mathbb Z/(q\mathbb Z)\rightarrow \mathbb Z/(q\mathbb Z), x\mapsto x+1 and \mu is the averaged counting measure. Let v:\mathbb Z/(q\mathbb Z)\rightarrow \mathbb R, hence A^{(v)}:\mathbb Z/(q\mathbb Z)\rightarrow SL(2,\mathbb R).

For any A:\mathbb Z/(q\mathbb Z)\rightarrow SL(2,\mathbb R), we have for any j, A_q(j+1)A(j)=A(j)A_q(j). This implies that

-the eigenvalue \tau(A_q(j), u_q(j)) of A_q(j) is independent of j. Denote it by \tau(A_q, u_q).
L(A)=\frac{1}{q}\ln\delta(A_q).

Here for any bounded linear operator A on any Banach space, \delta(A)=\lim\limits_{n\rightarrow\infty}\|A^n\|^{\frac{1}{n}}=\inf_{n\leq1}\|A^n\|^{\frac{1}{n}} is the spectral radius of A.  From the above facts we get

L(A)+i2\pi\rho(A)=\frac{1}{q}\ln\tau(A_q,u_q).

We also have the following obvious equivalent relations

L(A)>0\Leftrightarrow |trA_q|>2\Leftrightarrow (f,A)\in\mathcal U\mathcal H and  |trA_q|<2\Leftrightarrow Elliptic,

where tr stands for trace. For the second case we also have tr(A_q)=2\cos(2\pi \rho(A)q).

Back to Schrodinger case, there is a nice graph of the function \psi(E)=trA^{(E-v)}_q. (which is also 2\cos(2\pi\rho(E)q) for elliptic case). It’s obviously a polynomial in E of degree q. It has exactly q-1 critical points with critical values y satisfying |y|\geq2. We have in fact the following description of the spectrum \Sigma of the correponding operator H_v

Theorem: \Sigma consists of q bands and there are q-1 spectral gaps ( bands may touch at the boundary points, or equivalently, gap may collapse).

Proof: By the same argument for Schrodinger cocycle over fixed point above and the fact \rho(AB)=\rho(A)+\rho(B), we have the following easy facts for \rho(E) as a function on real line:

-it’s continuous on \mathbb R and is analytic in the interior of spectrum;
-it’s \frac{k}{2q}-valued outside the interior of spectrum thus constant in each connected components of the resolvent set;
\rho(-\infty)=\frac{1}{2} and \rho(\infty)=0 and nonincreasing.

These together implies that:

\psi^{-1}[-2,2] consists of q compact intervals. Some of them may touch at the boundary points. These are spectrum bands. \rho'(E)<0 on \psi^{-1}(-2,2);
-between each two bands is the so-called spectrum gap and there are q-1 of them (some of them may collasped). On each of them \rho(E)=\frac{k}{2q},k=q-1,\cdots,1. These are labelings of spectral gaps. \square

The proof obviously implies the properties of the polynomial \psi(E).

A natural question is that when are all gaps open (not collapsed). Obviously by the proof of Theorem, all gaps are open if and only if all the roots of polynomials \psi(E)-2, \psi(E)+2 are simple. Let’s give another description of these polynomials. Let’s restrict the operator H_v to l^2(\mathbb Z/(q\mathbb Z)) with three different type of boundary conditions. Let u\in l^2(\mathbb Z/(q\mathbb Z))

1. First let’s restrict to any subinterval [j,j+n-1]\subset[0,q-1] and consider Dirichlet boundary condition, i.e. u(j-1)=u(j+n)=0. Denote it by H^{n}_{v,j}. In this case it can be represented as a n\times n symmetric matrix

H^{n}_{v,j}=\begin{pmatrix}v(j)&1&0&0\\1&v(j+1)&1&\vdots\\ 0&1&v(j+2)&\vdots\\ 0&0&1&\vdots\\\vdots&\vdots&0&1\\\vdots&\vdots&\vdots&v(j+n-1)\end{pmatrix}

Let \det(H^{n}_{v,j}-E)=P_n(j,E). Then by induction it’s easy to see that

A^{(v-E)}_n(j)=\begin{pmatrix}P_n(j,E)&-P_{n-1}(j+1,E)\\P_{n-1}(j,E)&-P_{n-2}(j+1,E)\end{pmatrix}.

Hence \psi(E)=P_{q}(0,E)-P_{q-2}(1,E). In case 2 and 3 we will only restrict to [0,q-1].

2. Periodic boundary condition, i.e. u(-1)=u(q-1), u(q)=u(0). Denote it by H^{p}_v, then it is

H^{p}_v=\begin{pmatrix}v(0)&1&0&1\\1&v(1)&1&0\\ 0&1&v(2)&\vdots\\ 0&0&1&0\\ 0&\vdots&0&1\\1&0&\vdots&v(q-1)\end{pmatrix}

3. Antipeiodic boundary condition, i.e. u(-1)=-u(q-1), u(q)=-u(0). Denote it by H^{a}_v, then it is

H^{a}_v=\begin{pmatrix}v(0)&1&0&-1\\1&v(1)&1&0\\ 0&1&v(2)&\vdots\\ 0&0&1&0\\ 0&\vdots&0&1\\-1&0&\vdots&v(q-1)\end{pmatrix}

Then by case 1 it’s not difficult to see that for some integer l,

\psi(E)-2=\begin{cases}\det(H^{p}_v-E)&\text{ if }q=2l\\\det(H^{a}_v-E)&\text{ if }q=2l-1\end{cases} and \psi(E)+2=\begin{cases}\det(H^{a}_v-E)&\text{ if } q=2l\\\det(H^{p}_v-E)&\text{ if } q=2l-1\end{cases}.

Thus all the spectral gaps are open if and only if all eigenvalues of the operators H^{p}_v and H^{a}_v are simple. An easy case is that assume v(j), j=0,\cdots,q-1 are sufficiently large and distinct. Then after scaling, all nondigonal coefficients of H^{p}_v and H^{a}_v are sufficiently small. Namely, H^{p}_v and H^{a}_v are small perturbation of digonal matrices with distinct eigenvalues. Then so are H^{p}_v and H^{a}_v themself. Which implies that all gaps are open.

For simplicity, consider q even. Denote eigenvalues of H^{p}_v by \mu_1<\cdots<\mu_q and H^{a}_v by \lambda_1<\cdots<\lambda_q. Then spectrum bands are

[\mu_j,\lambda_j], j odd; [\lambda_j,\mu_j], j even.

And spectral gaps are

(\mu_j,\mu_{j+1}), j even; (\lambda_j,\lambda_{j+1}), j odd.

Finally let’s consider L(E)+i2\pi\rho(E):\mathbb H\rightarrow\mathbb C. Then it’s easy to see that it can be analytically extends through interior of each bands and through gaps. But they cannot be globally defined, since there are nontrivial winding of the invariant direction u_q(E) around each \mu_j, \lambda_j. This winding comes from the parabolicity. Indeed, if we instead consider the eigenvalue \lambda(E) of A^{(E-v)}_q, then

\frac{1}{q}\ln\lambda(E)=L(E)+i2\pi\rho(E) and \lambda(E)=\frac{1}{2}(\psi(E)\pm\sqrt{\psi(E)^2-4}),

of which the derivative has singularity at parabolicity. This also explain why L(E) and \rho(E) as functions on the whole real line can at most be \frac{1}{2}-H\ddot older continous.

Note for periodic potential and in spectrum bands, it’s always L(E)=0 since they are just parabolic and elliptic matrices. Thus by Theorem 2 of Notes 4, all the spectrum are purely absolutely continous.

Assume potentials are uniformly bounded. Then it’s interesting to note that as q\rightarrow\infty, there are more and more bands which are also thiner and thiner. Thus in quasiperiodic potential case, it’s natural to expect the spectrum is Cantor set under some assumption. We will give an example in next post.

Advertisements

Leave a Comment »

No comments yet.

RSS feed for comments on this post. TrackBack URI

Leave a Reply

Fill in your details below or click an icon to log in:

WordPress.com Logo

You are commenting using your WordPress.com account. Log Out / Change )

Twitter picture

You are commenting using your Twitter account. Log Out / Change )

Facebook photo

You are commenting using your Facebook account. Log Out / Change )

Google+ photo

You are commenting using your Google+ account. Log Out / Change )

Connecting to %s

Blog at WordPress.com.

%d bloggers like this: