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CASINO manual - Theory of Condensed Matter

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22.3 The RPA form <strong>of</strong> the u term<br />

An alternative to the u term described above is the common RPA form, which in casino has been<br />

implemented as<br />

u RPA<br />

ij = − A ( [1 − exp − r )]<br />

ij<br />

, (158)<br />

r ij F<br />

in three dimensions, where A and F are variational parameters. In two dimensions, the equivalent<br />

expression is<br />

u RPA<br />

ij = −√ A ( [1 − exp − r √ )]<br />

ij<br />

rij 2F − rij<br />

. (159)<br />

F<br />

The usual polynomial cut<strong>of</strong>f function is applied to these terms. This alters the cusp conditions, which<br />

are, in three dimensions,<br />

A(F ) = 2L uΓ ij F 2<br />

L u + 2CF , (160)<br />

and in two dimensions,<br />

A(F ) = 3L uΓ ij F 3/2<br />

L u + 3CF , (161)<br />

where Γ ij = 1/4 if i and j are electrons <strong>of</strong> the same spin, and Γ ij = 1/2 if their spins are different. If i<br />

and j are particles other than electrons, the value <strong>of</strong> Γ ij will also depend on their masses and charges.<br />

Note that in two-dimensional bilayer systems, where electrons <strong>of</strong> different spins are on separate layers,<br />

the anti-parallel cusp conditions are lifted, and the antiparallel A is a free parameter.<br />

The RPA u term is rarely used in practice, as the polynomial u term generally gives lower variational<br />

energies.<br />

22.4 The p and q terms in the Jastrow factor<br />

The p term takes the cuspless form<br />

p(r ij ) = ∑ A<br />

∑<br />

a A cos(G A · r ij ) , (162)<br />

G + A<br />

where the {G A } are the reciprocal lattice vectors <strong>of</strong> the simulation cell belonging to the Ath star <strong>of</strong><br />

vectors that are equivalent under the full symmetry group <strong>of</strong> the Bravais lattice, and ‘+’ means that,<br />

if G A is included in the sum, −G A is excluded. The p term is important if the finite-size correction<br />

to the kinetic energy is to be calculated (see Sec. 29).<br />

For systems with inversion symmetry the q term takes the cuspless form<br />

q(r i ) = ∑ ∑<br />

b B cos(G B · r i ), (163)<br />

B<br />

G + B<br />

where the {G B } are the reciprocal lattice vectors <strong>of</strong> the primitive unit cell belonging to the Bth star<br />

<strong>of</strong> vectors that are equivalent under the space-group symmetry <strong>of</strong> the crystal, and the ‘+’ means that,<br />

if G B is included in the sum, −G B is excluded. The q term is rarely <strong>of</strong> use in practice.<br />

22.5 The three-body W term<br />

The W term is given by<br />

W =<br />

N∑<br />

¯δ jk¯δjl¯δkl s lj · s lk , (164)<br />

j,k,l<br />

s jk = w jk r jk , (165)<br />

where w jk = w(r jk ) is a suitably parametrized function <strong>of</strong> the distance between electrons j and k,<br />

r jk = r j − r k , and the symbol ¯δ jk (no-delta <strong>of</strong> j, k) is short-hand for 1 − δ jk .<br />

The core function w ij is parametrized in casino as<br />

w ij = w(r ij ) = f C (r ij ; L w )<br />

148<br />

n∑<br />

c l rij l . (166)<br />

l=0

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