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<Strong>Goal:</Strong> we will introduce the Anderson model, discuss the behaviour as a function of the dimension. In 1d localization can be connected to the product of random matrices.
'''Goal.''' We introduce the Anderson model and study the statistical properties of its eigenstates.
In one dimension disorder leads to localization of all eigenstates, which can be understood using products of random matrices.


= Anderson model (tight binding model)=  
= Anderson model (tight-binding model) =


We consider disordered non-interacting particles hopping between nearest neighbors  sites on a lattice. The hamiltonian reads:
We consider non-interacting particles hopping between nearest-neighbour sites of a lattice in the presence of disorder.
<center> <math>
H= - t \sum_{ <i, j> } (c_i^\dagger c_j +c_j^\dagger c_i) \sum_i V_i c_i^\dagger c_i
</math></center>
The single particle hamiltonian in 1d reads
<center> <math>
H =
\begin{bmatrix}
V_1 & -t & 0 & 0 & 0 & 0 \\
-t & V_2 & -t & 0 & 0 & 0 \\
0 & -t & V_3 & -t & 0 & 0 \\
0 & 0  & -t & \ldots &-t & 0\\
0 & 0  & 0  & -t & \ldots & -t\\
0 & 0  & 0  & 0 & -t & V_L
\end{bmatrix}
</math></center>


For simplicity we set the hopping <math>t=1 </math>. The disorder are iid random variables drawn, uniformly from the box <math>(-\frac{W}{2},\frac{W}{2})</math>.
The Hamiltonian reads


The final goal is to study the statistical properties of eigensystem
<math display="block">
<center> <math>
H =
H \psi=\epsilon \psi, \quad \text{with} \sum_{n=1}^L |\psi_n|^2=1
- t \sum_{\langle i,j\rangle} (c_i^\dagger c_j + c_j^\dagger c_i)
</math></center>
+
\sum_i V_i c_i^\dagger c_i .
</math>
 
The random variables <math>V_i</math> represent on-site disorder.
 
For simplicity we set
 
<math>t=1</math>.
 
The disorder variables are independent random variables drawn from the box distribution
 
<math display="block">
V_i \in \left(-\frac{W}{2},\frac{W}{2}\right).
</math>
 
In one dimension the single-particle Hamiltonian corresponds to a tridiagonal matrix
 
<math display="block">
H =
\begin{pmatrix}
V_1 & -1 & 0 & 0 & \dots \\
-1 & V_2 & -1 & 0 & \dots \\
0 & -1 & V_3 & -1 & \dots \\
0 & 0 & -1 & \ddots & -1 \\
\dots & \dots & \dots & -1 & V_L
\end{pmatrix}.
</math>
 
We study the statistical properties of the eigenvalue problem
 
<math display="block">
H\psi = \epsilon \psi ,
\qquad
\sum_{n=1}^L |\psi_n|^2 = 1 .
</math>
 
---
 
== Density of states ==
 
Without disorder the dispersion relation is
 
<math display="block">
\epsilon(k) = -2\cos k,
\qquad
k\in(-\pi,\pi).
</math>


== Density of states (DOS)==
The energy band is therefore


In 1d and in absence of disorder, the dispersion relation is
<math display="block">
<math> \epsilon(k) = -2 \cos k, \quad  k \in  (-\pi, \pi), -2< \epsilon(k)< 2 </math>. From the dispersion relation, we compute the density of states (DOS) :
-2 < \epsilon < 2 .
<center><math>
</math>
\rho(\epsilon) =\int_{-\pi}^\pi \frac{d k}{2 \pi} \delta(\epsilon-\epsilon(k))=\frac{1}{\pi } \frac{1}{\sqrt{4-\epsilon^2}} \quad \text{for } \epsilon \in (-2,2)</math></center>


In presence of disorder the DOS becomes larger, and display sample to sample fluctuations. One can consider its mean value, avergaed  over disorder realization.
The density of states is


==Transfer matrices and Lyapunov exponents==
<math display="block">
\rho(\epsilon)
=
\int_{-\pi}^{\pi}
\frac{dk}{2\pi}
\delta(\epsilon-\epsilon(k))
=
\frac{1}{\pi\sqrt{4-\epsilon^2}}
\qquad
(\epsilon\in(-2,2)).
</math>


In the presence of disorder the density of states broadens and becomes sample dependent.


== Product of random matrices==
---


Let's consider again the Anderson Model in 1d. The eigensystem is well defined in a box of size L with Dirichelet boundary condition on the extremeties of the box.
== Transfer matrices ==


Here we will solve the second order differential equation imposing instead Cauchy boundaries on one side of the box. Let's rewrite the previous eigensystem in the following form
The discrete Schrödinger equation reads
<center> <math>
 
\begin{bmatrix}
<math display="block">
\psi_{n+1} + \psi_{n-1} + V_n \psi_n = \epsilon \psi_n .
</math>
 
It can be rewritten as
 
<math display="block">
\begin{pmatrix}
\psi_{n+1} \\
\psi_{n+1} \\
\psi_{n}
\psi_n
\end{bmatrix}
\end{pmatrix}
=
=
\begin{bmatrix}
T_n
V_n -\epsilon & -1 \\
\begin{pmatrix}
1 & 0
\psi_n \\
\end{bmatrix}  \begin{bmatrix}
\psi_{n} \\
\psi_{n-1}
\psi_{n-1}
\end{bmatrix}
\end{pmatrix}
</math></center>
</math>
We can continue the recursion
 
<center> <math>
with
\begin{bmatrix}
 
\psi_{n+1} \\
<math display="block">
\psi_{n}
T_n =
\end{bmatrix}
\begin{pmatrix}
=
V_n-\epsilon & -1 \\
\begin{bmatrix}
V_n -\epsilon & -1 \\
1 & 0
1 & 0
\end{bmatrix}  \begin{bmatrix}
\end{pmatrix}.
V_{n-1} -\epsilon & -1 \\
</math>
1 & 0
 
\end{bmatrix} \begin{bmatrix}
Iterating gives
\psi_{n-1} \\
 
\psi_{n-2}
<math display="block">
\end{bmatrix}
\begin{pmatrix}
</math></center>
It is useful to introduce the transfer matrix and their product
<center> <math>
T_n =\begin{bmatrix}
V_n -\epsilon & -1 \\
1 & 0
\end{bmatrix},  \quad \Pi_n= T_n \cdot T_{n-1} \cdot\ldots T_1
</math></center>
The Schrodinger equation can  be written as
<center> <math>
\begin{bmatrix}
\psi_{n+1} \\
\psi_{n+1} \\
\psi_{n}
\psi_n
\end{bmatrix}
\end{pmatrix}
=
=
\Pi_n \begin{bmatrix}
\Pi_n
\psi_{1} \\
\begin{pmatrix}
\psi_{0}
\psi_1 \\
\end{bmatrix}
\psi_0
\end{pmatrix},
\qquad
\Pi_n = T_n T_{n-1} \cdots T_1 .
</math>
 
Thus the wavefunction is controlled by a product of random matrices.
 
---
 
== Lyapunov exponent ==
 
Define
 
<math display="block">
\|\Pi_n\|^2 =
\frac{\pi_{11}^2+\pi_{12}^2+\pi_{21}^2+\pi_{22}^2}{2}.
</math>
 
Furstenberg's theorem ensures
 
<math display="block">
\lim_{n\to\infty}
\frac{1}{n}\ln\|\Pi_n\|
=
=
\begin{bmatrix}
\gamma .
\pi_{11} & \pi_{12} \\
</math>
\pi_{21} &  \pi_{22}
 
\end{bmatrix}  \begin{bmatrix}
The quantity <math>\gamma</math> is the Lyapunov exponent.
\psi_{1} \\
 
\psi_{0}
Without disorder
\end{bmatrix}
 
</math></center>
<math display="block">
==== Fustenberg Theorem ====
\gamma=0
We define the norm of a 2x2 matrix:
\qquad (\epsilon\in(-2,2)).
<center> <math>
</math>
\|\Pi_n\|^2 =\frac{\pi_{11}^2+\pi_{21}^2+\pi_{12}^2+\pi_{22}^2}{2}
 
</math></center>
For generic disorder
For large N, the Fustenberg theorem ensures the existence of the non-negative Lyapunov exponent, namely
<center> <math>
\lim_{n\to \infty}  \frac{\ln \|\Pi_n\|}{n} = \gamma \ge 0
</math></center>
In absence of disorder <math> \gamma =0 </math> for <math>\epsilon \in (-2,2)</math>. Generically the Lyapunov is positive, <math> \gamma >0 </math>, and depends on <math>\epsilon </math> and on the distribution of <math>V_i </math>.


====Consequences====
<math display="block">
\gamma>0 .
</math>


<Strong> Localization length</Strong>
---


Together with the norm, also  <math> |\psi_n|^2</math> grows exponentially with n. We can write
== Localization length ==
<center>  <math>
\ln |\psi_n|  \sim \gamma n + \gamma_2 \chi \sqrt{n}</math>
</center>
which means that <math> \ln |\psi_n| </math> is performing a random walk with a drift.


The transfer-matrix recursion corresponds to fixing the wavefunction at one boundary and propagating it through the system.


However, our initial goal is a properly normalized eigenstate at energy <math>\epsilon </math>. We need  to switch from  Cauchy, where you set the initial condition, to Dirichelet or vonNeuman, where you set the behaviour at  the two boundaries. The true eigenstate is obtained by matching two "Cauchy" solutions on the half box and imposing the normalization. Hence, we obtain a localized eigenstate  and we can identify
Typical solutions grow exponentially
<center> <math>  
 
\xi_{\text{loc}}(\epsilon)  \equiv  \gamma^{-1}(\epsilon)
<math display="block">
|\psi_n|\sim e^{\gamma n}.
</math>
</math>
</center>


However a physical eigenstate must satisfy boundary conditions at both ends of the system. Matching two such solutions leads to exponentially localized eigenstates


<Strong> Fluctuations</Strong>
<math display="block">
|\psi_n|\sim e^{-|n-n_0|/\xi_{\text{loc}}}.
</math>
 
The localization length is
 
<math display="block">
\xi_{\text{loc}}(\epsilon)=\frac{1}{\gamma(\epsilon)}.
</math>
 
Thus in one dimension arbitrarily weak disorder localizes all eigenstates. 
This result is consistent with the scaling theory of localization discussed earlier, which predicts that for <math>d\le2</math> disorder inevitably drives the system toward the insulating regime.
 
---
 
== Fluctuations ==
 
Quantities such as
 
<math>
|\psi_n|,\quad \|\Pi_n\|,\quad G
</math>
 
show strong sample-to-sample fluctuations, while their logarithm is self-averaging.
 
For instance
 
<math display="block">
\ln|\psi_n|
\sim
\gamma n + O(\sqrt n)
</math>


We expect strong fluctuations on quantites like <math> |\psi_n|, \|\Pi_n\|, G, \ldots </math>, while their logarithm is self averaging.
so that the logarithm of the wavefunction performs a random walk with a positive drift.

Latest revision as of 21:39, 12 March 2026

Goal. We introduce the Anderson model and study the statistical properties of its eigenstates. In one dimension disorder leads to localization of all eigenstates, which can be understood using products of random matrices.

Anderson model (tight-binding model)

We consider non-interacting particles hopping between nearest-neighbour sites of a lattice in the presence of disorder.

The Hamiltonian reads

H=ti,j(cicj+cjci)+iVicici.

The random variables Vi represent on-site disorder.

For simplicity we set

t=1.

The disorder variables are independent random variables drawn from the box distribution

Vi(W2,W2).

In one dimension the single-particle Hamiltonian corresponds to a tridiagonal matrix

H=(V11001V21001V3100111VL).

We study the statistical properties of the eigenvalue problem

Hψ=ϵψ,n=1L|ψn|2=1.

---

Density of states

Without disorder the dispersion relation is

ϵ(k)=2cosk,k(π,π).

The energy band is therefore

2<ϵ<2.

The density of states is

ρ(ϵ)=ππdk2πδ(ϵϵ(k))=1π4ϵ2(ϵ(2,2)).

In the presence of disorder the density of states broadens and becomes sample dependent.

---

Transfer matrices

The discrete Schrödinger equation reads

ψn+1+ψn1+Vnψn=ϵψn.

It can be rewritten as

(ψn+1ψn)=Tn(ψnψn1)

with

Tn=(Vnϵ110).

Iterating gives

(ψn+1ψn)=Πn(ψ1ψ0),Πn=TnTn1T1.

Thus the wavefunction is controlled by a product of random matrices.

---

Lyapunov exponent

Define

Πn2=π112+π122+π212+π2222.

Furstenberg's theorem ensures

limn1nlnΠn=γ.

The quantity γ is the Lyapunov exponent.

Without disorder

γ=0(ϵ(2,2)).

For generic disorder

γ>0.

---

Localization length

The transfer-matrix recursion corresponds to fixing the wavefunction at one boundary and propagating it through the system.

Typical solutions grow exponentially

|ψn|eγn.

However a physical eigenstate must satisfy boundary conditions at both ends of the system. Matching two such solutions leads to exponentially localized eigenstates

|ψn|e|nn0|/ξloc.

The localization length is

ξloc(ϵ)=1γ(ϵ).

Thus in one dimension arbitrarily weak disorder localizes all eigenstates. This result is consistent with the scaling theory of localization discussed earlier, which predicts that for d2 disorder inevitably drives the system toward the insulating regime.

---

Fluctuations

Quantities such as

|ψn|,Πn,G

show strong sample-to-sample fluctuations, while their logarithm is self-averaging.

For instance

ln|ψn|γn+O(n)

so that the logarithm of the wavefunction performs a random walk with a positive drift.