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TRANSCRIPT
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Lecture XVII 49
Lecture XVII: Weakly Interacting Electron Gas: Plasma Theory
How are the properties of an electron gas influenced by weak Coulomb interaction?
Qualitative considerations:
When is the intereaction weak? Defining r0 =1
n1/3as the average electron separation,
the typical p.e. e2
r0and k.e.
2
mr0lead to the dimensionless ratio, rs =
e2
r0
mr202
r0a0
, where
a0 is electron Bohr radius, from which one can infer that Coulomb effects dominate atlow density
At rs 35 there is (believed to be) a transition to an electron solid phaseknown as a Wigner crystal (cf. Mott-Hubbard insulator)
For most metals (2 < rs < 6), k.e. and p.e. comparable; fortunately (thanks toadiabatic continuity) weak coupling theory valid even for intermediate rs
Motivates consideration of weak coupling theory rs 1: -convention on spin
H =
ddr c(r)
p2
2mc(r) +
1
2
ddr
ddrc(r)c
(r
)e2
|r r|c(r
)c(r)
Aim: to explore dielectric properties and ground state energy of electron gas through...
Quantum partition function: using CSPI formulation
Z tr e(HN) =
(0)=()(0)=()
D(, )eS[,]
S[, ] =
0
d
ddr (r, )
+
p2
2m
(r, )
+1
2
ddr
ddr(r, )(r
, )e2
|r r|(r
, )(r, )
Expressed in Fourier basis: (r, ) =1L3
k,n
ei(krn)k,n,
S =
0
d
k
k() ( + k ) k() +1
2Ld
q=0
4e2
q2q()q()
where k =2k2
2mand q() =
ddr eiqr(r, )
k k()k+q,()
(N.B. neutralising background exclusion of q = 0 from sum)
With the action quartic in fermionic fields , Z can not be evaluated exactly
For weak interaction, rs 1, we could expand in Coulomb interaction: Feynman diagram expansion (cf. Gell-MannBruckner theory)
Lecture Notes October 2005
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Lecture XVII 50
Alternative use field integral to isolate leading diagrammatic series expansion
known as the Random Phase Approximation (RPA)
General principle:
When confronted with interacting field theory, seek decomposition of interactionthrough introduction of auxiliary field which captures low-energy content of theory
In some cases, these fields are identified with the elementary particles that mediatethe interaction (see below); in others, these fields encode the low-energy collective modesof the system (e.g. superfluid, superconductor)
Decoupling facilitated using the Hubbard-Stratonovich transformation:
eR0 d
Pq=0
2e2
Ldq2q()q() =
D e
R0 d
Pq=0
q2
8 q()q()+ie
2Ld/2(q()q()+q()q())
Physically, represents (scalar) photon field which mediates Coulomb interactionN.B. real and periodic ( + ) = ()
Z =
D(, )
D exp
0
d
ddr
1
8()2 +
+
p2
2m + ie
Gaussian in Grassmann fields, field integral may be performed:
using identity D[, ] exp[M ] = detM = exp[ln detM]Z =
D exp
0
d
ddr
1
8()2 +
spin2 ln det
+
p2
2m + ie
Setting e = 0, photon field decouples from determinant;
recovers partition function of non-interacting electron gas
Perturbation Theory in e:
Define free particle Green function: G0 = [ +p2
2m ]1
and expand:ln(1 + x) =
n=1(x)
n/n
lndet
+
p2
2m + ie
trln
G10 + ie
= tr ln G10 + tr ln
1 + ieG0
= tr ln G10 tr
ieG0 +
1
2
ieG0
2+
First order term: for convenience, set k (k, n), etc.
2tr[G0] = 2k
G0(k) k|G0|k
1L3k=0 k||k =
2L3
k
1
in + k 0 = 0
Lecture Notes October 2005
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Lecture XVII 51
0 = 0 due to neutralising background
Second order term:
2 e2
2tr[G0]
2 = e2k,q
G0(k) k|G0|k
1L3
q k||k + q
G0(k + q) k + q|G0|k + q
1L3
q k + q||k=
e2
2
q
(q)qq
where density-density response function,
(q) =2
L3 k1
in + k
1
in im + k+q
Combined with bare term, to leading order in e2 (Random Phase Approximation),
Z = Z0
D eS[], S[] =
1
2
q
D1(q) q2
4 e2(q)
|q|
2 + O(e4)
Z0 denotes partition function of non-interacting gas
Physically, D1(q) denotes dynamically screened Coulomb interaction
D1(q) = (q)q2
4, (q) = 1
4e2
q2(q)
where (q) is the energy and momentum dependent effective dielectric function
mq,
4e 2
q2
k,n
m
n
+
+k+q,
mq,( )
=
-1
mq,=
=
++ ...
+
Diagrammatic interpretation:
D(q) =4
q21
1 4e2
q2(q)
=4
q2
n=0
e2(q)
4
q2
n
Lecture Notes October 2005