**Computational Physics II FYS4411/FYS9411**, Department of Physics, University of Oslo, Norway

Date: **Jan 11, 2019**

Copyright 1999-2019, Computational Physics II FYS4411/FYS9411. Released under CC Attribution-NonCommercial 4.0 license

The aim of this project is to use the Variational Monte Carlo (VMC) method to evaluate the ground state energy, onebody densities, expectation values of the kinetic and potential energies and single-particle denisties of quantum dots with $N=2$, $N=6$, $N=12$ and $N=20$ electrons. These are so-called closed shell systems.

We consider a system of electrons confined in a pure two-dimensional isotropic harmonic oscillator potential, with an idealized total Hamiltonian given by

$$
\begin{equation}
\label{eq:finalH} \tag{1}
\hat{H}=\sum_{i=1}^{N} \left( -\frac{1}{2} \nabla_i^2 + \frac{1}{2} \omega^2r_i^2 \right)+\sum_{i<j}\frac{1}{r_{ij}},
\end{equation}
$$

$$
\hat{H}_0=\sum_{i=1}^{N} \left( -\frac{1}{2} \nabla_i^2 + \frac{1}{2} \omega^2r_i^2 \right),
$$

and the repulsive interaction between two electrons given by

$$
\hat{H}_1=\sum_{i<j}\frac{1}{r_{ij}},
$$

with the distance between electrons given by $r_{ij}=\vert \boldsymbol{r}_1-\boldsymbol{r}_2\vert$. We define the modulus of the positions of the electrons (for a given electron $i$) as $r_i = \sqrt{r_{i_x}^2+r_{i_y}^2}$.

In exercises a-f we will deal only with a system of
two electrons in a quantum dot with a frequency of $\hbar\omega = 1$.
The reason for this is that we have exact closed form expressions
for the ground state energy from Taut's work for selected values of $\omega$,
see M. Taut, Phys. Rev. A **48**, 3561 (1993).
The energy is given by $3$ a.u. (atomic units) when the interaction between the electrons is included.
If only the harmonic oscillator part of the Hamiltonian is included,
the so-called unperturbed part,

$$
\hat{H}_0=\sum_{i=1}^{N} \left( -\frac{1}{2} \nabla_i^2 + \frac{1}{2} \omega^2r_i^2 \right),
$$

$$
\phi_{n_x,n_y}(x,y) = A H_{n_x}(\sqrt{\omega}x)H_{n_y}(\sqrt{\omega}y)\exp{(-\omega(x^2+y^2)/2}.
$$

The functions $H_{n_x}(\sqrt{\omega}x)$ are so-called Hermite polynomials, discussed in connection with project 1 while $A$ is a normalization constant. For the lowest-lying state we have $n_x=n_y=0$ and an energy $\epsilon_{n_x,n_y}=\omega(n_x+n_y+1) = \omega$. Convince yourself that the lowest-lying energy for the two-electron system is simply $2\omega$.

The unperturbed wave function for the ground state of the two-electron system is given by

$$
\Phi(\boldsymbol{r}_1,\boldsymbol{r}_2) = C\exp{\left(-\omega(r_1^2+r_2^2)/2\right)},
$$

with $C$ being a normalization constant and $r_i = \sqrt{r_{i_x}^2+r_{i_y}^2}$. Note that the vector $\boldsymbol{r}_i$ refers to the $x$ and $y$ position for a given particle. What is the total spin of this wave function? Find arguments for why the ground state should have this specific total spin.

We want to perform a Variational Monte Carlo calculation of the ground state of two electrons in a quantum dot well with different oscillator energies, assuming total spin $S=0$ using the Hamiltonian of Eq. (1). Our trial wave function which has the following form

$$
\begin{equation}
\psi_{T}(\boldsymbol{r}_1,\boldsymbol{r}_2) =
C\exp{\left(-\alpha\omega(r_1^2+r_2^2)/2\right)}
\exp{\left(\frac{ar_{12}}{(1+\beta r_{12})}\right)},
\label{eq:trial} \tag{2}
\end{equation}
$$

where $a$ is equal to one when the two electrons have anti-parallel spins and $1/3$ when the spins are parallel. Finally, $\alpha$ and $\beta$ are our variational parameters. Note well the dependence on $\alpha$ for the single-particle part of the trial function. It is important to remember this when you use higher-order Hermite polynomials. Find the analytical expressions for the local energy.

Your task is to perform a Variational Monte Carlo calculation using the Metropolis algorithm to compute the integral

$$
\begin{equation}
\langle E \rangle =
\frac{\int d\boldsymbol{r}_1d\boldsymbol{r}_2\psi^{\ast}_T(\boldsymbol{r}_1,\boldsymbol{r}_2)\hat{H}(\boldsymbol{r}_1,\boldsymbol{r}_2)\psi_T(\boldsymbol{r}_1,\boldsymbol{r}_2)}
{\int d\boldsymbol{r}_1d\boldsymbol{r}_2\psi^{\ast}_T(\boldsymbol{r}_1,\boldsymbol{r}_2)\psi_T(\boldsymbol{r}_1,\boldsymbol{r}_2)}.
\label{_auto1} \tag{3}
\end{equation}
$$

Compute the expectation value of the energy using both the analytical expression for the local energy and numerical derivation of the kinetic energy. Compare the time usage between the two approaches. Perform these calculations without importance sampling and also without the Jastrow factor. For the calculations without the Jastrow factor and repulsive Coulomb potential, your energy should equal 2.0 a.u. and your variance should be exactly equal to zero.

Add now importance sampling and repeat the calculations from the previous exercise but use only the analytical expression for the local energy. Perform also a blocking analysis in order to obtain the optimal standard deviation. Compare your results with the those without importance sampling and comment your results.

Using either the steepest descent method or the conjugate gradient method, find the optimal variational
parameters and perform your Monte Carlo calculations using these.

In addition, you should parallelize your program using MPI and set it up to run on Smaug.

Finally, we wil now analyze and interpret our results for the two-electron systems. Find the energy minimum and discuss your results compared with the analytical solution from Taut's work, see reference [1] below. Compute also the mean distance $r_{12}=\vert \boldsymbol{r}_1-\boldsymbol{r}_2\vert$ (with $r_i = \sqrt{r_{i_x}^2+r_{i_y}^2}$) between the two electrons for the optimal set of the variational parameters. With the optimal parameters for the ground state wave function, compute the onebody density. Discuss your results and compare the results with those obtained with a pure harmonic oscillator wave functions. Run a Monte Carlo calculations without the Jastrow factor as well and compute the same quantities. How important are the correlations induced by the Jastrow factor? Compute also the expectation value of the kinetic energy and potential energy using $\omega=0.01$, $\omega=0.05$, $\omega=0.1$, $\omega=0.5$ and $\omega=1.0$. Comment your results. Hint, think of the virial theorem.

Discuss also your results with those obtained with Hartree-Fock theory for two electrons from project 1.

The previous exercises have prepared you for extending your calculational machinery to other systems. Here we will focus on quantum dots with $N=6$ and $N=12$ electrons.

The new item you need to pay attention to is the calculation of the Slater Determinant. This is an additional complication
to your VMC calculations.

If we stick to harmonic oscillator like wave functions,
the trial wave function for say an $N=6$ electron quantum dot can be written as

$$
\begin{equation}
\psi_{T}(\boldsymbol{r}_1,\boldsymbol{r}_2,\dots, \boldsymbol{r}_6) =
Det\left(\phi_{1}(\boldsymbol{r}_1),\phi_{2}(\boldsymbol{r}_2),
\dots,\phi_{6}(\boldsymbol{r}_6)\right)
\prod_{i<j}^{6}\exp{\left(\frac{a r_{ij}}{(1+\beta r_{ij})}\right)},
\label{_auto2} \tag{4}
\end{equation}
$$

$$
\begin{equation}
\psi_{T}(\boldsymbol{r}_1,\boldsymbol{r}_2, \dots,\boldsymbol{r}_{12}) =
Det\left(\phi_{1}(\boldsymbol{r}_1),\phi_{2}(\boldsymbol{r}_2),
\dots,\phi_{12}(\boldsymbol{r}_{12})\right)
\prod_{i<j}^{12}\exp{\left(\frac{ar_{ij}}{(1+\beta r_{ij})}\right)},
\label{_auto3} \tag{5}
\end{equation}
$$

In this case you need to include the $n_x=2$ and $n_y=2$ wave functions as well. Observe that $r_i = \sqrt{r_{i_x}^2+r_{i_y}^2}$. Use the Hermite polynomials defined in project 1. Reference [5] gives benchmark results for closed-shell systems up to $N=20$.

Write a function which sets up the Slater determinant. Find the Hermite polynomials which are needed for $n_x=0,1,2$ and obviously $n_y$ as well. Compare the results you obtain with those from project 1. Compute the ground state energies of quantum dots for $N=6$ and $N=12$ electrons, following the same set up as in the previous exercises for $\omega=0.01$, $\omega=0.05$, $\omega=0.1$, $\omega=0.5$, and $\omega=1.0$. The calculations should include parallelization, blocking, importance sampling and energy minimization using the conjugate gradient approach or similar approaches. To test your Slater determinant code, you should reproduce the unperturbed single-particle energies when the electron-electron repulsion is switched off. Convince yourself that the unperturbed ground state energies for $N=6$ is $10\omega$ and for $N=12$ we obtain $28\omega$. What is the expected total spin of the ground states?

With the optimal parameters for the ground state wave function, compute again the onebody density. Discuss your results and compare the results with those obtained with a pure harmonic oscillator wave functions. Run a Monte Carlo calculations without the Jastrow factor as well and compute the same quantities. How important are the correlations induced by the Jastrow factor? Compute also the expectation value of the kinetic energy and potential energy using $\omega=0.01$, $\omega=0.05$, $\omega=0.1$, $\omega=0.5$, and $\omega=1.0$. Comment your results.

The last exercise is a performance analysis of your code(s) for the case of $N=6$ electrons. Make a performance analysis by timing your serial code with and without vectorization. Perform several runs with the same number of Monte carlo cycles and compute an average timing analysis with and without vectorization. Comment your results. Use at least $10^6$ Monte Carlo samples.

Compare thereafter your serial code(s) with the speedup you get by parallelizing your code, running either OpenMP or MPI or both. Do you get a near $100\%$ speedup with the parallel version? Comment again your results and perform timing benchmarks several times in order to extract an average performance time.

M. Taut, Phys. Rev. A

**48**, 3561 - 3566 (1993).B. L. Hammond, W. A. Lester and P. J. Reynolds,

*Monte Carlo methods in Ab Initio Quantum Chemistry*, World Scientific, Singapore, 1994, chapters 2-5 and appendix B.B. H. Bransden and C. J. Joachain, Physics of Atoms and molecules, Longman, 1986. Chapters 6, 7 and 9.

A. K. Rajagopal and J. C. Kimball, see Phys. Rev. B

**15**, 2819 (1977).M. L. Pedersen, G. Hagen, M. Hjorth-Jensen, S. Kvaal, and F. Pederiva, Phys. Rev. B

**84**, 115302 (2011)

Here follows a brief recipe and recommendation on how to write a report for each project.

Give a short description of the nature of the problem and the eventual numerical methods you have used.

Describe the algorithm you have used and/or developed. Here you may find it convenient to use pseudocoding. In many cases you can describe the algorithm in the program itself.

Include the source code of your program. Comment your program properly.

If possible, try to find analytic solutions, or known limits in order to test your program when developing the code.

Include your results either in figure form or in a table. Remember to label your results. All tables and figures should have relevant captions and labels on the axes.

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Critique: if possible include your comments and reflections about the exercise, whether you felt you learnt something, ideas for improvements and other thoughts you've made when solving the exercise. We wish to keep this course at the interactive level and your comments can help us improve it.

Try to establish a practice where you log your work at the computerlab. You may find such a logbook very handy at later stages in your work, especially when you don't properly remember what a previous test version of your program did. Here you could also record the time spent on solving the exercise, various algorithms you may have tested or other topics which you feel worthy of mentioning.

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