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Numerical Renormalization Group Calculations for Impurity ...

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3.3. Flow diagrams and Fixed points 27<br />

basis {|ψ (N)<br />

n 〉}.<br />

H 0 =<br />

H 1 =<br />

.<br />

.<br />

.<br />

H N =<br />

H N+1 =<br />

∑N s<br />

n=1<br />

∑N s<br />

n=1<br />

∑N s<br />

n=1<br />

∑N s<br />

n=1<br />

E (0)<br />

n |ψ(0) n 〉〈ψ(0) n |<br />

E (1)<br />

n |ψ (1)<br />

n 〉〈ψ (1)<br />

n |<br />

E (N)<br />

n<br />

E (N+1)<br />

n<br />

|ψ n<br />

(N) 〉〈ψ n (N) |<br />

|ψ n<br />

(N+1) 〉〈ψ n (N+1) | (3.60)<br />

where H m |ψ (m)<br />

n<br />

〉 = E (m)<br />

n<br />

|ψ (m)<br />

n 〉, (m = 0, 1, ..., N + 1 and n = 1, ..., N s ).<br />

The iterative Hamiltonian H N approaches to the fixed point H ∗ as the eigenstates<br />

{|ψ (N)<br />

n 〉} converges to constant states {|ψ ∗ n 〉}:<br />

lim<br />

N→∞ |ψ(N) n 〉 = |ψ∗ n 〉, (3.61)<br />

<strong>for</strong> n = 1, ..., N s .<br />

Once the iterative Hamiltonian is very close to a fixed point, the mapping R<br />

hardly affects the structure of Hamiltonian but changes the overall energy-scale<br />

as α. 9<br />

A sequence of trans<strong>for</strong>mations gives<br />

H N+1 = R α (H N ) = α H N + O(1/N)<br />

H N+2<br />

H N+3<br />

= R α (H N+1 ) = α 2 H N + O(1/N)<br />

= R α (H N+2 ) = α 3 H N + O(1/N)<br />

... (3.62)<br />

If we define an renormalized Hamiltonian ¯H N where overall energy scale is divided<br />

by α N , ( ¯H N = H N × 1<br />

α N )<br />

¯H N+1 = ¯H N + O(1/N)<br />

¯H N+2 = ¯H N + O(1/N)<br />

¯H N+3 = ¯H N + O(1/N)<br />

9 In fermionic (bosonic) NRG, α = 1/ √ Λ (1/Λ).<br />

... (3.63)

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