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Problem set 2 for the physics 216: many-body theory course offered in the spring of 2002. The problem set includes four questions covering topics such as green's functions, cooper pair size, superconductivity, and a tight-binding-like model. Students are asked to calculate fourier-transformed green's functions, estimate cooper pair size and rotational velocity, check commutation relations, and solve a tight-binding-model problem.
Typology: Exercises
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iGrαβ (t 1 , r 1 , t 2 , r 2 ) =
{ 〈Ψα(t 1 , r 1 )Ψ† β (t 2 , r 2 ) + Ψ† β (t 2 , r 2 )Ψα(t 1 , r 1 )〉 if t 1 − t 2 > 0 0 if t 1 − t 2 < 0.
Calculate the Fourier-transformed Green’s function Gr(ω, p) for the free Fermi gas at temperature T (i.e., the expectation value 〈〉 is taken with respect to the finite-temperature Fermi gas). Be sure to specify where any poles occur. Check that contour integration of your result indeed gives zero for negative t = t 1 − t 2.
ξ ∼
¯hvF ∆
What is the order of magnitude of the rotational velocity of one He atom in a pair? You may wish to use the fact that the effective mass is m∗^ = 3. 1 m.
Compare the rotational velocity to the Fermi velocity, which you can estimate by recalling that the effective mass m∗^ = 3. 1 m and knowing that the Fermi momentum is pF = ¯h(0. 8 × 108 cm−^1 ).
Reversing the diagonalization, what does this say about the expectation values of pairs of the original Ψ operators? In particular, can there be a nonzero expectation value in the BCS state of “anomalous” combinations of operators like Ψ†(t 1 , r 1 )Ψ†(0, 0) that vanish in the normal state?
H = −t
∑
〈ij〉,σ
(ciσc† jσ + h.c.) −
∑
i
Uini↑ni↓ (3)
The first sum is over nearest-neighbor pairs.
Suppose that U is positive (so that there is an attractive interaction whenever two particles are on the same site) and weak compared to the hopping t. Also suppose that the system is at half-filling (one electron per site on average). Start by solving the U = 0 problem. Then calculate the Vkk′ matrix elements induced by U that should appear in the pairing Hamiltonian as functions of t. What do you expect to be the angular momentum of the Cooper pairs? (i.e., s-wave, p-wave, etc.) Estimate the transition temperature in terms of the original parameters of the model.