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My PhD thesis - Condensed Matter Theory - Imperial College London

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CHAPTER 7. THE ELECTRONIC GROUND-STATE WAVE FUNCTION<br />

FROM CLASSICAL PLASMON NORMAL MODES<br />

where<br />

M kk ′ = ˆk · ˆk ′ ∫<br />

V<br />

V<br />

ω 2 p(r)e i(k−k′ )·r) d 3 r. (7.25)<br />

The reason for choosing opposite signs in the transforms of f and ρ is to ensure that<br />

f k and ρ k are conjugate variables. This conjugate variable requirement implies that<br />

ρ k = ∂L({f k}, { f ˙ k })<br />

∂ ˙<br />

∫<br />

=<br />

V<br />

= 1 √<br />

V<br />

∫<br />

f k<br />

δL[f, f] ˙<br />

δf(r, ˙ t)<br />

V<br />

∂ ˙ f(r, t)<br />

∂ ˙ f k<br />

d 3 r<br />

ρ(r, t)e ik·r d 3 r. (7.26)<br />

The k = 0 terms are excluded; this will be the case for all sums from now on. The<br />

justification for this is that the average charge density fluctuation is constrained to<br />

be zero, and the average potential (which corresponds to ˙ f k=0 ) may be chosen to be<br />

zero.<br />

7.2 Quantisation and diagonalisation of the Hamiltonian<br />

In equation (7.24), the Hamiltonian is expressed in terms of pairs of discrete conjugate<br />

variables.<br />

subject to the commutation relation<br />

Quantisation proceeds by letting f k and ρ k become operators,<br />

[ ]<br />

ρk , f k ′ = −iδkk ′. (7.27)<br />

These are not Hermitian operators; however, they are the Fourier components of<br />

operators corresponding to real, observable fields, and must obey the symmetry<br />

rules<br />

ρ † k = ρ −k, f † k = f −k. (7.28)<br />

The quantum-mechanical Hamiltonian operator is therefore<br />

H = 1 ∑<br />

(<br />

)<br />

ρ † δ kk ′<br />

k<br />

2 ɛ<br />

k,k ′ 0 k ρ 2 k ′ + ɛ 0f k kM kk ′k ′ f † k<br />

. (7.29)<br />

′<br />

111

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