Carsten Timm: Theory of superconductivity
Carsten Timm: Theory of superconductivity
Carsten Timm: Theory of superconductivity
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10<br />
BCS theory<br />
The variational ansatz <strong>of</strong> Sec. 9.2 has given us an approximation for the many-particle ground state |ψ BCS ⟩. While<br />
this is interesting, it does not yet allow predictions <strong>of</strong> thermodynamic properties, such as the critical temperature.<br />
We will now consider superconductors at non-zero temperatures within mean-field theory, which will also provide<br />
a new perspective on the BCS gap equation and on the meaning <strong>of</strong> ∆ k .<br />
10.1 BCS mean-field theory<br />
We start again from the Hamiltonian<br />
H = ∑ kσ<br />
ξ k c † kσ c kσ + 1 N<br />
∑<br />
kk ′ V kk ′ c † k↑ c† −k,↓ c −k ′ ,↓c k′ ↑. (10.1)<br />
A mean-field approximation consists <strong>of</strong> replacing products <strong>of</strong> operators A, B according to<br />
Note that the error introduced by this replacement is<br />
AB ∼ = ⟨A⟩ B + A ⟨B⟩ − ⟨A⟩ ⟨B⟩ . (10.2)<br />
AB − ⟨A⟩ B − A ⟨B⟩ + ⟨A⟩ ⟨B⟩ = (A − ⟨A⟩)(B − ⟨B⟩), (10.3)<br />
i.e., it is <strong>of</strong> second order in the deviations <strong>of</strong> A and B from their averages. A well-known mean-field approximation<br />
is the Hartree or Stoner approximation, which for our Hamiltonian amounts to the choice A = c † k↑ c k ′ ↑, B =<br />
c † −k,↓ c −k ′ ,↓. However, Bardeen, Cooper, and Schrieffer realized that <strong>superconductivity</strong> can be understood with<br />
the help <strong>of</strong> a different choice, namely A = c † k↑ c† −k,↓ , B = c −k ′ ,↓c k′ ↑. This leads to the mean-field BCS Hamiltonian<br />
H BCS = ∑ ξ k c † kσ c kσ + 1 ∑ (<br />
)<br />
V kk ′ ⟨c † k↑<br />
N<br />
c† −k,↓ ⟩ c −k ′ ,↓c k′ ↑ + c † k↑ c† −k,↓ ⟨c −k ′ ,↓c k′ ↑⟩ − ⟨c † k↑ c† −k,↓ ⟩⟨c −k ′ ,↓c k′ ↑⟩ .<br />
kσ<br />
kk ′ (10.4)<br />
We define<br />
∆ k := − 1 ∑<br />
V kk ′ ⟨c −k<br />
N<br />
′ ,↓c k ′ ↑⟩ (10.5)<br />
k ′<br />
so that<br />
∆ ∗ k = − 1 ∑<br />
V kk ′ ⟨c † k<br />
N<br />
′ ↑ c† −k ′ ,↓⟩. (10.6)<br />
k ′<br />
At this point it is not obvious that the quantity ∆ k is the same as the one introduced in Sec. 9.2 for the special<br />
case <strong>of</strong> the ground state. Since this will turn out to be the case, we nevertheless use the same symbol from the<br />
start. We can now write<br />
H BCS = ∑ kσ<br />
ξ k c † kσ c kσ − ∑ k<br />
∆ ∗ k c −k,↓ c k↑ − ∑ k<br />
∆ k c † k↑ c† −k,↓<br />
+ const. (10.7)<br />
89