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@ -1332,11 +1332,11 @@ gfortran hydrogen.f90 qmc_stats.f90 qmc_uniform.f90 -o qmc_uniform
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$$ \mathbf{r}_0 \rightarrow \mathbf{r}_1 \rightarrow \mathbf{r}_2 \ldots \mathbf{r}_{N_{\rm MC}}\,, $$
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according to the following algorithm.
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following the following algorithm.
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At every step, we propose a new move according to a transition probability $T(\mathbf{r}_{n+1},\mathbf{r}_n)$ of our choice.
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At every step, we propose a new move according to a transition probability $T(\mathbf{r}_{n}\rightarrow\mathbf{r}_{n+1})$ of our choice.
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For simplicity, let us move the electron in a 3-dimensional box of side $2\delta L$ centered at the current position
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For simplicity, we will move the electron in a 3-dimensional box of side $2\delta L$ centered at the current position
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of the electron:
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$$
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@ -1347,19 +1347,19 @@ gfortran hydrogen.f90 qmc_stats.f90 qmc_uniform.f90 -o qmc_uniform
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$\mathbf{u}$ is a uniform random number in a 3-dimensional box
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$(-1,-1,-1) \le \mathbf{u} \le (1,1,1)$.
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After having moved the electron, add the
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After having moved the electron, we add the
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accept/reject step that guarantees that the distribution of the
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$\mathbf{r}_n$ is $\Psi^2$. This amounts to accepting the move with
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probability
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$$
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A{\mathbf{r}_{n+1},\mathbf{r}_n) = \min\left(1,\frac{T(\mathbf{r}_{n},\mathbf{r}_{n+1}) P(\mathbf{r}_{n+1})}{T(\mathbf{r}_{n+1},\mathbf{r}_n)P(\mathbf{r}_{n})}\right)\,,
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A{\mathbf{r}_{n}\rightarrow\mathbf{r}_{n+1}) = \min\left(1,\frac{T(\mathbf{r}_{n},\mathbf{r}_{n+1}) P(\mathbf{r}_{n+1})}{T(\mathbf{r}_{n+1},\mathbf{r}_n)P(\mathbf{r}_{n})}\right)\,,
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$$
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which, for our choice of transition probability, becomes
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$$
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A{\mathbf{r}_{n+1},\mathbf{r}_n) = \min\left(1,\frac{P(\mathbf{r}_{n+1})}{P(\mathbf{r}_{n})}\right)= \min\left(1,\frac{\Psi(\mathbf{r}_{n+1})^2}{\Psi(\mathbf{r}_{n})^2}
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A{\mathbf{r}_{n}\rightarrow\mathbf{r}_{n+1}) = \min\left(1,\frac{P(\mathbf{r}_{n+1})}{P(\mathbf{r}_{n})}\right)= \min\left(1,\frac{\Psi(\mathbf{r}_{n+1})^2}{\Psi(\mathbf{r}_{n})^2}
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$$
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Explain why the transition probability cancels out in the expression of $A$. Also note that we do not need to compute the norm of the wave function!
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@ -1394,7 +1394,8 @@ gfortran hydrogen.f90 qmc_stats.f90 qmc_uniform.f90 -o qmc_uniform
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possible, keeping the number of accepted steps not too small. To
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achieve that, we define the acceptance rate as the number of
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accepted steps over the total number of steps. Adjusting the time
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step such that the acceptance rate is close to 0.5 is a good compromise for the current problem.
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step such that the acceptance rate is close to 0.5 is a good
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compromise for the current problem.
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*** Exercise
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@ -1697,18 +1698,18 @@ end subroutine random_gauss
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probability of transition from $\mathbf{r}_n$ to
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$\mathbf{r}_{n+1}$.
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In the previous example, we were using uniform random
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numbers. Hence, the transition probability was
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In the previous example, we were using uniform sampling in a box centered
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at the current position. Hence, the transition probability was symmetric
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\[
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T(\mathbf{r}_{n} \rightarrow \mathbf{r}_{n+1}) =
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T(\mathbf{r}_{n} \rightarrow \mathbf{r}_{n+1}) = T(\mathbf{r}_{n+1} \rightarrow \mathbf{r}_{n})
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\text{constant}\,,
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\]
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so the expression of $A$ was simplified to the ratios of the squared
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wave functions.
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Now, if instead of drawing uniform random numbers we
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Now, if instead of drawing uniform random numbers, we
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choose to draw Gaussian random numbers with zero mean and variance
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$\delta t$, the transition probability becomes:
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@ -1718,10 +1719,10 @@ end subroutine random_gauss
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\mathbf{r}_{n+1} - \mathbf{r}_{n} \right)^2}{2\delta t} \right]\,.
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\]
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To sample even better the density, we can "push" the electrons
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Furthermore, to sample the density even better, we can "push" the electrons
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into in the regions of high probability, and "pull" them away from
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the low-probability regions. This will mechanically increase the
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the low-probability regions. This will ncrease the
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acceptance ratios and improve the sampling.
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To do this, we can use the gradient of the probability density
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@ -1730,8 +1731,18 @@ end subroutine random_gauss
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\frac{\nabla [ \Psi^2 ]}{\Psi^2} = 2 \frac{\nabla \Psi}{\Psi}\,,
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\]
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and add the so-called drift vector, so that the numerical scheme becomes a drifted diffusion:
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and add the so-called drift vector, so that the numerical scheme becomes a
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drifted diffusion with transition probability:
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\[
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T(\mathbf{r}_{n} \rightarrow \mathbf{r}_{n+1}) =
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\frac{1}{(2\pi\,\delta t)^{3/2}} \exp \left[ - \frac{\left(
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\mathbf{r}_{n+1} - \mathbf{r}_{n} - \frac{\nabla
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\Psi(\mathbf{r}_n)}{\Psi(\mathbf{r}_n)} \right)^2}{2\,\delta t} \right]\,.
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\]
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and the corrsponding move is proposed as
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\[
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\mathbf{r}_{n+1} = \mathbf{r}_{n} + \delta t\, \frac{\nabla
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\Psi(\mathbf{r})}{\Psi(\mathbf{r})} + \chi \,,
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@ -1739,18 +1750,11 @@ end subroutine random_gauss
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where $\chi$ is a Gaussian random variable with zero mean and
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variance $\delta t$.
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The transition probability becomes:
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\[
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T(\mathbf{r}_{n} \rightarrow \mathbf{r}_{n+1}) =
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\frac{1}{(2\pi\,\delta t)^{3/2}} \exp \left[ - \frac{\left(
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\mathbf{r}_{n+1} - \mathbf{r}_{n} - \frac{\nabla
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\Psi(\mathbf{r}_n)}{\Psi(\mathbf{r}_n)} \right)^2}{2\,\delta t} \right]\,.
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\]
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The algorithm of the previous exercise is only slighlty modified summarized:
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The algorithm of the previous exercise is only slighlty modified as:
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0) For the starting position compute $\Psi$ and the drif-vector $\frac{\nabla \Psi(\mathbf{r})}{\Psi(\mathbf{r})}$
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1) Compute a new position $\mathbf{r'} = \mathbf{r}_n +
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\delta t\, \frac{\nabla \Psi(\mathbf{r})}{\Psi(\mathbf{r})} + \chi$
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@ -1813,8 +1817,8 @@ end subroutine drift
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*** Exercise 2
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#+begin_exercise
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Modify the previous program to introduce the drifted diffusion scheme.
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(This is a necessary step for the next section).
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Modify the previous program to introduce the drift-diffusion scheme.
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(This is a necessary step for the next section on diffusion Monte Carlo).
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#+end_exercise
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*Python*
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@ -2076,10 +2080,10 @@ gfortran hydrogen.f90 qmc_stats.f90 vmc_metropolis.f90 -o vmc_metropolis
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Consider the time-dependent Schrödinger equation:
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\[
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i\frac{\partial \Psi(\mathbf{r},t)}{\partial t} = \hat{H} \Psi(\mathbf{r},t)
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i\frac{\partial \Psi(\mathbf{r},t)}{\partial t} = \hat{H} \Psi(\mathbf{r},t)\,.
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\]
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We can expand $\Psi(\mathbf{r},0)$, in the basis of the eigenstates
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We can expand a given starting wave function, $\Psi(\mathbf{r},0)$, in the basis of the eigenstates
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of the time-independent Hamiltonian:
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\[
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@ -2092,17 +2096,17 @@ gfortran hydrogen.f90 qmc_stats.f90 vmc_metropolis.f90 -o vmc_metropolis
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\Psi(\mathbf{r},t) = \sum_k a_k \exp \left( -i\, E_k\, t \right) \Phi_k(\mathbf{r}).
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\]
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Now, let's replace the time variable $t$ by an imaginary time variable
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Now, if we replace the time variable $t$ by an imaginary time variable
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$\tau=i\,t$, we obtain
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\[
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-\frac{\partial \psi(\mathbf{r}, \tau)}{\partial \tau} = \hat{H} \psi(\mathbf{r}, \tau)
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\]
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where $\psi(\mathbf{r},\tau) = \Psi(\mathbf{r},-i\tau) = \Psi(\mathbf{r},t)$
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where $\psi(\mathbf{r},\tau) = \Psi(\mathbf{r},-i\,)$
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and
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\[
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\psi(\mathbf{r},\tau) = \sum_k a_k \exp( -E_k\, \tau) \phi_k(\mathbf{r}).
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\psi(\mathbf{r},\tau) = \sum_k a_k \exp( -E_k\, \tau) \phi_k(\mathbf{r}).
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\]
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For large positive values of $\tau$, $\psi$ is dominated by the
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$k=0$ term, namely the lowest eigenstate.
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