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My PhD thesis - Condensed Matter Theory - Imperial College London

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CHAPTER 3.<br />

QUANTUM MONTE CARLO METHODS<br />

3.1 Random sampling<br />

To calculate expectation values of observables in quantum mechanics, we need to<br />

evaluate expressions of the form:<br />

∫<br />

Ψ<br />

∗ 〈Ô〉 = (X)ÔΨ(X) dX<br />

∫<br />

Ψ∗ (X)Ψ(X) dX , (3.1)<br />

where<br />

Ô is a Hermitian operator and X is a vector representing all the electron<br />

coordinates.<br />

For large systems, the dimension of the integrals is correspondingly large. Computation<br />

of such integrals by conventional quadrature methods becomes impractical,<br />

because the error in these calculations scales poorly in high dimensions. For example,<br />

the error in a Simpson’s Rule calculation scales as M −4/d , where M is the<br />

number of grid points and d is the dimensionality of the integral. As d increases,<br />

improving the accuracy of the calculation becomes prohibitively expensive.<br />

In contrast, the Monte Carlo method of integration generates a statistical error<br />

in the value of the integral which scales as M −1/2 , independent of the dimension.<br />

While this is worse than grid-based techniques when d is small, it is far superior for<br />

large d.<br />

One way of evaluating the integral<br />

∫<br />

I = g(r) dr (3.2)<br />

Ω<br />

is to sample a set of M random vectors {r i } from a distribution which is uniform over<br />

the region of integration Ω. Each vector is assigned a score g(r i ) and the integral is<br />

estimated as<br />

I ≈ Ω M<br />

M∑<br />

g(r i ). (3.3)<br />

i=1<br />

This is the Monte Carlo method of integration, and in this form, it is not very<br />

efficient. It can be much improved by using importance sampling. The integral is<br />

first rewritten as<br />

∫<br />

I =<br />

f(r)P (r) dr, (3.4)<br />

31

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