20.02.2014 Views

Numerical Renormalization Group Calculations for Impurity ...

Numerical Renormalization Group Calculations for Impurity ...

Numerical Renormalization Group Calculations for Impurity ...

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

2.2. Quantum phase transitions and quantum critical points 7<br />

with which the Hamiltonian in Eq. (2.18) is written in a diagonal <strong>for</strong>m of<br />

H I (g) = ∑ k<br />

ε k (g)(γ † k γ k − 1/2). (2.20)<br />

The diagonal <strong>for</strong>m in Eq. (2.20) is obtained using the two consequent trans<strong>for</strong>mations<br />

of the Jordan-Wigner trans<strong>for</strong>mation 3 and the Bogolioubov trans<strong>for</strong>mation.<br />

4<br />

The ground state, |0〉, of H I (g) has no γ fermions and there<strong>for</strong>e satisfies<br />

γ k |0〉 = 0 <strong>for</strong> all k. The excited states are created by occupying the singleparticle<br />

states; they can clearly be classified by the total number of occupied<br />

states and a n-particle state has the <strong>for</strong>m γ † k 1<br />

γ † k 2<br />

...γ † k n<br />

|0〉, with all the k i distinct.<br />

The energy gap between the ground state and the first excited one occurs at<br />

k = 0 and equals<br />

∆(g) = 2J(1 − g). (2.21)<br />

There<strong>for</strong>e the model H I (g) exhibits a quantum phase transition at the critical<br />

coupling g = 1, which separates an ordered state with Z 2 symmetry broken (g ≪<br />

1) from a quantum paramagnetic state where the symmetry remains unbroken<br />

(g ≫ 1). The state at g = 1 is critical and there is a universal continuum quantum<br />

field theory that describes the critical properties in its vicinity.<br />

We shall now obtain the critical theory <strong>for</strong> the model in Eq. (2.18). We define<br />

the continuum Fermi field<br />

Ψ(x) = 1 √ a<br />

c i , (2.22)<br />

that satisfies<br />

{Ψ(x), Ψ † (x ′ )} = δ(x − x ′ ). (2.23)<br />

To express H I (g) in terms of Ψ and the expansions in spatial gradients yields the<br />

continuum H F ,<br />

∫<br />

H F = E 0 +<br />

[ ]<br />

c<br />

dx<br />

2 (Ψ†∂Ψ† ∂x − Ψ∂Ψ ∂x ) + ∆Ψ† Ψ + ..., (2.24)<br />

where the ellipses represent terms with higher gradients, and E 0 is an uninteresting<br />

additive constant. The coupling constant in H F are<br />

∆ = 2J(1 − g), c = 2Ja. (2.25)<br />

Notice that at the critical point g = 1, we have ∆ = 0, and we have ∆ > 0 in the<br />

magnetically ordered phase and ∆ < 0 in the quantum paramagnet.<br />

3 To map the Hamiltonian H I (g) with spin-1/2 degrees of freedom into a quadratic ones with<br />

the spinless Fermi operators<br />

4 To trans<strong>for</strong>m the quadratic Hamiltonian into a <strong>for</strong>m whose number is conserved.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!