CASINO manual - Theory of Condensed Matter
CASINO manual - Theory of Condensed Matter
CASINO manual - Theory of Condensed Matter
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where n αβ (r, r ′ ) is the charge density <strong>of</strong> the N β −δ αβ electrons <strong>of</strong> spin β calculated with an electron <strong>of</strong><br />
spin α held fixed at r. We can now average g αβ (r, r ′ ) over the surface <strong>of</strong> a sphere <strong>of</strong> radius ρ centred<br />
on r. The vector r ′ − r can be written in spherical polar coordinates as (ρ, θ, φ). The required pair<br />
correlation function is then<br />
∫<br />
gαβ(r, F 1<br />
ρ) =<br />
4πρ 2 g αβ (r, r ′ ) δ(|r ′ − r| − ρ) dΩ, (355)<br />
where dΩ = sin θ dθ dφ. This gives<br />
∫<br />
gαβ(r, F 1<br />
ρ) =<br />
4πρ 2 g αβ (r, r ′ ) δ(|r ′ − r| − ρ) dΩ (356)<br />
=<br />
∫<br />
1 |Ψ F | 2 ∑ N β −δ αβ<br />
j=1 δ(|r j,β − r ′ | − ρ) dr 2 . . . dr N<br />
∫<br />
4πρ 2 dΩ. (357)<br />
|ΨF | 2 dr 2 . . . dr N n β (r ′ )<br />
This type <strong>of</strong> averaging was used by Maezono et al. [83]. The pair correlation functions can be evaluated<br />
in ρ bins for each r <strong>of</strong> interest. Equations (347), (349) and (357) contain one or two charge densities<br />
in the denominator. When one or both <strong>of</strong> these charge densities is very small there will be a large<br />
amount <strong>of</strong> noise in the quantity evaluated. We expect g αβ (r, r ′ ) to tend to 1 − δ αβ /N β as r − r ′<br />
becomes large, while for small values <strong>of</strong> r − r ′ we expect it be less than one. One strategy for coping<br />
with the noise would be to set a lower limit on the charge density n β (r ′ ) below which the contribution<br />
to Eq. (357) is not accumulated.<br />
33.3.5 Collecting in bins<br />
Assume the system is homogeneous and isotropic. The pair correlation function g αβ (r) can be collected<br />
in bins <strong>of</strong> width ∆, giving<br />
g αβ (r n ) = Ω 〈 N<br />
n 〉<br />
αβ<br />
, (358)<br />
Ω n N α N β<br />
where Nαβ n is the number <strong>of</strong> α, β-spin pairs whose separation falls within the nth bin (the pairs iα, jα<br />
and jα, iα should be counted separately, and similarly for the parallel β-spins), and Ω n is the volume<br />
<strong>of</strong> the nth bin. Note that if we consider a single bin, so that Ω = Ω n , then Nαβ n = N α(N β − δ αβ ).<br />
This confirms that the normalization <strong>of</strong> Eq. (358) is correct, but note that our formulae disagree with<br />
Eq. (35) <strong>of</strong> Ortiz and Ballone [84].<br />
The volume <strong>of</strong> the nth bin, Ω n , is given by<br />
Ω n = 4 3 π ( n 3 − (n − 1) 3) ∆ 3 = 4π ( n 2 − n + 1/3 ) ∆ 3 . (359)<br />
One could define r n to be the centre <strong>of</strong> the nth bin, but a better choice is [85]<br />
r n = 3∆ 4<br />
[n 4 − (n − 1) 4 ]<br />
[n 3 − (n − 1) 3 ] = 3∆ 4<br />
[4n 3 − 6n 2 + 4n − 1]<br />
[3n 2 . (360)<br />
− 3n + 1]<br />
If g were to be linear across each bin and if g were sampled exactly without statistical error then Eqs.<br />
(358) and (359) would reproduce the exact value at each point r n .<br />
In two dimensions one requires the area <strong>of</strong> the nth circular strip,<br />
A n = π((n∆) 2 − ((n − 1)∆) 2 ) = π∆ 2 (2n − 1). (361)<br />
We want to average f(r) = ar + b over a strip, and find the corresponding radius r n . Therefore<br />
Hence<br />
f(r n ) =<br />
r n = 2∆ 3<br />
∫ n∆<br />
(n−1)∆<br />
f(r) 2πr dr<br />
∫ n∆<br />
2πr dr<br />
(n−1)∆<br />
= [ 1 3 ar3 + 1 2 br2 ] n∆<br />
(n−1)∆<br />
[ 1 2 r2 ] n∆<br />
(n−1)∆<br />
= a 2[(n∆)3 − ((n − 1)∆) 3 ]<br />
3[(n∆) 2 − ((n − 1)∆) 2 ] + b<br />
= ar n + b.<br />
[n 3 − (n − 1) 3 ]<br />
[n 2 − (n − 1) 2 ] = 2∆ 3<br />
[3n 2 − 3n + 1]<br />
. (362)<br />
[2n − 1]<br />
190