Numerical Renormalization Group Calculations for Impurity ...
Numerical Renormalization Group Calculations for Impurity ...
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)