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CASINO manual - Theory of Condensed Matter

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large and the wave function is near zero are not sampled at all in a VMC run. The subsequent<br />

optimization run then has no incentive to keep the wave function near zero and produces large<br />

fluctuations in the corresponding coefficients, thus severely degrading the wave function.<br />

• Only the optimization <strong>of</strong> coefficients has been tested successfully. The optimization <strong>of</strong> exponents<br />

and primitive corrections remains to be explored.<br />

7.4.7 Free orbitals and pairing wave functions<br />

There are four basic different types <strong>of</strong> pairing orbitals available in casino, and any linear combination<br />

<strong>of</strong> them is allowed. In the following, r represents the vector between the particles being paired,<br />

r = r i − r j .<br />

• The plane-wave pairing orbital is<br />

N pw<br />

∑<br />

φ(r) = p l exp(ik l · r) , (3)<br />

l=1<br />

where the optimizable parameters are the linear p l coefficients. The k l vectors are the reciprocal<br />

lattice vectors <strong>of</strong> the simulation cell. Notice that the coefficients for all plane waves in<br />

the same star are constrained to be the same (they need not be supplied more than once in<br />

correlation.data).<br />

• The Gaussian pairing orbital is<br />

N g<br />

∑<br />

φ(r) = α l exp(−β l r 2 ) , (4)<br />

l=1<br />

where α l and β l are the optimizable parameters. One can optionally constrain the parameters<br />

so that they correspond to the Gaussian expansion <strong>of</strong> an exponential,<br />

φ(r) ≈ exp (−r/R ex ) , (5)<br />

in which case R ex is the only optimizable parameter, and the α l and β l are varied accordingly.<br />

• The polynomial pairing orbital is<br />

( ) Cp N<br />

Lp − r ∑ p<br />

φ(r) =<br />

a n r n , (6)<br />

L p<br />

where N p and C p are the order and truncation order <strong>of</strong> the polynomials, respectively, L p is the<br />

cut<strong>of</strong>f radius and a n are the polynomial coefficients.<br />

n=0<br />

• The Slater pairing orbital is<br />

∑N S<br />

φ(r) = c s exp<br />

(− a sr 2 )<br />

∑N P<br />

+ (C p · r) exp<br />

(− A pr 2 )<br />

1 + b s r<br />

1 + B p r<br />

s=1<br />

p=1<br />

(7)<br />

where N S and N P are the orders <strong>of</strong> the S-type and P-type expansions, respectively, and c s , a s ,<br />

b s , C p , A p and B p are optimizable parameters.<br />

If more than one <strong>of</strong> these forms is defined inside the ‘PAIRING’ section <strong>of</strong> the ‘FREE ORBS’ block<br />

in correlation.data, they are added together to form the final orbital. In the following example all<br />

four forms are combined.<br />

START PAIRING<br />

Spin-pair dependence (CURRENTLY HAS NO EFFECT)<br />

0<br />

START PLANE-WAVE TERM<br />

Number <strong>of</strong> plane waves<br />

3<br />

Parameter ;<br />

Optimizable (0=NO; 1=YES)<br />

69

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