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My PhD thesis - Condensed Matter Theory - Imperial College London

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CHAPTER 9.<br />

ENERGY<br />

A NEW CALCULATION OF THE JELLIUM SURFACE<br />

-0.5<br />

-1<br />

-1.5<br />

-2<br />

ε slab (mHa)<br />

-2.5<br />

-3<br />

-3.5<br />

-4<br />

s = 11.7783<br />

-4.5<br />

s = 15.1317<br />

s = 18.4851<br />

-5<br />

0.005 0.01 0.015 0.02 0.025 0.03 0.035 0.04<br />

s/N<br />

Figure 9.6: The slab energy per electron, plotted against s/N, where s is the slab width and N is<br />

the number of electrons. The abscissa is proportional to 1/L 2 , and was chosen to demonstrate the<br />

form of the finite-size errors.<br />

imately as 1/L 2 . The reason that the Jastrow factor performs less well in small<br />

systems is almost certainly the parameter L c . This parameter, which keeps the<br />

wave function free of unwanted cusps, depends on the cell size, and is not allowed to<br />

be optimised. It modifies the long-range behaviour of the two-body term; it does not<br />

appear to affect the electron density adversely (by rendering the derived one-body<br />

term less efficient).<br />

Most importantly, this finite-size error is independent of the slab width: the<br />

evidence for this is the fact that the different curves in figure 9.6 remain equallyspaced.<br />

This allows an accurate calculation of the surface energy to be made.<br />

First, the curves s = 11.7783 and s = 15.1317 are interpolated on the abscissae<br />

of the third curve, s = 18.4851. Working with the largest possible system size<br />

(and thus effectively eliminating the Coulomb finite-size error), the slab energies<br />

per electron at this point are (in mHa) -3.713 ± 0.063, -4.060 ± 0.051 and -4.593<br />

177

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