Numerical Renormalization Group Calculations for Impurity ...
Numerical Renormalization Group Calculations for Impurity ...
Numerical Renormalization Group Calculations for Impurity ...
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3.2. Summary of the Basic Techniques 23<br />
The semi-infinite chain is solved iteratively by starting from H 0 and successively<br />
adding the next site.<br />
H 0 = H imp + √ ∑<br />
ξ 0 (f † −1σ f 0σ + f † 0σ f ∑<br />
−1σ) + ε 0 f † 0σ f 0σ<br />
H 1<br />
H 2<br />
H 3<br />
...<br />
H N+1<br />
σ<br />
∑<br />
∑<br />
= H 0 + t 0 (f 0σf † 1σ + f 1σf † 0σ ) + ε 1<br />
σ<br />
σ<br />
σ<br />
f † 1σf 1σ<br />
∑<br />
= H 1 + t 1 (f † 1σ f 2σ + f † 2σ f ∑<br />
1σ) + ε 2 f † 2σ f 2σ (3.35)<br />
σ<br />
∑<br />
∑<br />
= H 2 + t 2 (f 2σf † 3σ + f 3σf † 2σ ) + ε 3<br />
σ<br />
σ<br />
σ<br />
f † 3σf 3σ<br />
∑<br />
= H N + t N (f † Nσ f N+1σ + f † N+1σ f ∑<br />
Nσ) + ε N+1 f † N+1σ f N+1σ<br />
σ<br />
To prevent the rapid growth of the Hilbert space, it is indispensable to discard<br />
some of eigenstates be<strong>for</strong>e including an additional conduction site to the Hamiltonian.<br />
Let us assume that the Hamiltonian of the N −1-th iterative step, H N−1 ,<br />
yields M of eigenstates,<br />
H N−1 |φ (N−1)<br />
n<br />
〉 = E n<br />
(N−1) |φ n (N−1) 〉 (3.36)<br />
with n = 1, 2, ....M.<br />
The matrix representation of a new Hamiltonian H N is based on the product<br />
states<br />
|ψ nm (N) 〉 = |φ(N−1) n 〉 ⊗ |m〉, (n = 1, 2, ..., M, m = 1, 2, ..., l), (3.37)<br />
where {|m〉|m = 1, 2, ..., l} corresponds to a basis <strong>for</strong> a new site. In fermionic<br />
cases<br />
|Ω〉 = |0〉,<br />
| ↑〉 = f † N↑ |0〉,<br />
| ↓〉 = f † N↓ |0〉,<br />
The matrix elements of the new Hamiltonian H N is<br />
| ↑↓〉 = f † N↑ f † N↓<br />
|0〉. (3.38)<br />
σ<br />
〈ψ (N)<br />
n ′ m ′ |H N |ψ (N)<br />
nm 〉<br />
= 〈m ′ |m〉〈φ (N−1)<br />
n ′<br />
+ t N−1 〈φ (N−1)<br />
n ′<br />
|H N−1 |φ (N−1)<br />
n<br />
〉 + ε N 〈φ (N−1)<br />
n ′<br />
|f † N−1σ |φ(N−1) nσ 〉〈m ′ |f Nσ |m〉<br />
|φ n<br />
(N−1) 〉〈m ′ |f † Nσ f Nσ|m〉<br />
+ t N−1 〈φ (N−1)<br />
n<br />
|f ′ N−1σ |φ nσ (N−1) 〉〈m ′ |f † Nσ<br />
|m〉. (3.39)<br />
with |ψ (N−1)<br />
nm<br />
〉 = |φ n<br />
(N−1) 〉 ⊗ |m〉 and |m〉 ∈ {|Ω〉, | ↑〉, | ↓〉, | ↑↓〉}.<br />
In NRG, we truncate the matrix of Hamiltonian by keeping the first N s × N s<br />
elements out of the M × M ones and discarding the remnants.