My PhD thesis - Condensed Matter Theory - Imperial College London
My PhD thesis - Condensed Matter Theory - Imperial College London
My PhD thesis - Condensed Matter Theory - Imperial College London
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CHAPTER 4.<br />
ERRORS IN QMC SIMULATIONS<br />
Here M is the block length. If M is large enough, then successive values of Ōj will<br />
be uncorrelated; this occurs if M is greater than the correlation length of the data.<br />
The new error estimate is given by equation (4.25) with O i replaced by Ōi and N<br />
replaced by the number of blocks.<br />
If M is not sufficiently large then the blocking method gives an error estimate<br />
which is too small. Thus a way of determining the correct block length is to increase<br />
M until the calculated error reaches a plateau; this is then the best error estimate.<br />
This technique may not be possible if the correlation length is very long or there are<br />
insufficient sample points.<br />
In both VMC and DMC, the correlation length depends on the time step. If<br />
the time step is too small, then it takes many steps before a configuration changes<br />
significantly; however, if it is too large, then too many steps are rejected, and the<br />
time required to generate the next uncorrelated configuration is also large.<br />
4.4 Surface calculations<br />
There are several additional challenges which must must be met when dealing with<br />
surfaces, which will be detailed in the rest of this chapter.<br />
4.4.1 System geometry<br />
In order to study surfaces, it is usual to simulate slab systems (with two surfaces);<br />
using only a single surface creates problems with the boundary conditions.<br />
The aim is to model a slab with infinite extent in two dimensions, but the simulation<br />
cell must be finite; it is therefore normal to apply periodic boundary conditions<br />
to the cell. However, rather than applying these conditions in two dimensions, most<br />
surface calculations use fully three-dimensional periodicity. In addition, it is conventional<br />
to use the 3D version of the Ewald interaction; thus the system actually<br />
being simulated is a stack of slabs, as shown in figure 4.3.<br />
In density-functional and other mean-field calculations, this is not important.<br />
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