Modifs in conclusion

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Anthony Scemama 2020-08-03 18:15:34 +02:00
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@ -826,7 +826,7 @@ Searching for the optimal value of $\mu$ may be too costly, so we have
computed the MAD, MSE and RMSD for fixed values of $\mu$. The results
are illustrated in figure~\ref{fig:g2-dmc}. As seen on the figure and
in table~\ref{tab:mad}, the best choice for a fixed value of $\mu$ is
0.5~bohr$^{-1}$ for all three basis sets. Is is the value for which
0.5~bohr$^{-1}$ for all three basis sets. It is the value for which
the MAE (3.74(35), 2.46(18) and 2.06(35) kcal/mol) and RMSD (4.03(23),
3.02(06) and 2.74(13)~kcal/mol) are minimal. Note that these values
are even lower than those obtained with the optimal value of
@ -849,6 +849,19 @@ cancellations of errors.
The number of determinants in the trial wave functions are shown in
figure~\ref{fig:g2-ndet}. As expected, the number of determinants
is smaller when $\mu$ is small and larger when $\mu$ is large.
It is important to remark that the median of the number of
determinants when $\mu=0.5$~bohr$^{-1}$ is below 100~000 determinants
with the quadruple-zeta basis set, making these calculations feasilble
with such a large basis set. At the double-zeta level, compared to the
FCI trial wave functions the median of the number of determinants is
reduced by more than two orders of magnitude.
Moreover, going to $\mu=0.25$~bohr$^{-1}$ gives a median close to 100
determinants at the double-zeta level, and close to 1~000 determinants
at the quadruple-zeta level for only a slight increase of the
MAE. Hence, RS-DFT-CIPSI trial wave functions with small values of
$\mu$ could be very useful for large systems to go beyond the
single-determinant approximation at a very low computational cost
while keeping the size-consistency.
Note that when $\mu=0$ the number of determinants is not equal to one because
we have used the natural orbitals of a first CIPSI calculation, and
@ -872,10 +885,10 @@ on the determinant expansion is similar to the effect of re-optimizing
the CI coefficients in the presence of a Jastrow factor, but without
the burden of performing a stochastic optimization.
Varying the range-separation parameter $\mu$ and aproaching the
Varying the range-separation parameter $\mu$ and approaching the
RS-DFT-FCI with CIPSI provides a way to adapt the number of
determinants in the trial wave function, leading to size-consistent
FN-DMC energies.
determinants in the trial wave function, leading always to
size-consistent FN-DMC energies.
We propose two methods. The first one is for the computation of
accurate total energies by a one-parameter optimization of the FN-DMC
energy via the variation of the parameter $\mu$.
@ -883,12 +896,15 @@ The second method is for the computation of energy differences, where
the target is not the lowest possible FN-DMC energies but the best
possible cancellation of errors. Using a fixed value of $\mu$
increases the consistency of the trial wave functions, and we have found
that $\mu=0.5$~bohr${^-1}$ is the value where the cancellation of
that $\mu=0.5$~bohr$^{-1}$ is the value where the cancellation of
errors is the most effective.
Moreover, such a small value of $\mu$ gives extermely
compact wave functions, making this recipe a good candidate for
the accurate description of the whole potential energy surfaces of
large systems.
large systems. If the number of determinants is still too large, the
value of $\mu$ can be further reduced to $0.25$~bohr$^{-1}$ to get
extremely compact wave functions at the price of less efficient
cancellations of errors.
@ -906,31 +922,30 @@ Challenge 2019-gch0418) and from CALMIP (Toulouse) under allocation
\begin{enumerate}
\item Total energies and nodal quality:
\begin{itemize}
\item Facts: KS occupied orbitals closer to NOs than HF
\item Even if exact functional, complete basis set, still approximated nodes for KS
% \item Facts: KS occupied orbitals closer to NOs than HF
% \item Even if exact functional, complete basis set, still approximated nodes for KS
\item KS -> exponentially fast convergence (as HF) with basis because of non divergence of effective KS potential (citer le papier de Gill)
\item With correlation consistent basis set, FCI nodes (which include correlation) are better than KS
\item With FCI, good limit at CBS ==> exact energy
\item But slow convergence with basis set because of divergence of the e-e interaction not well represented in atom centered basis set
\item Exponential increase of number of Slater determinants
% \item With correlation consistent basis set, FCI nodes (which include correlation) are better than KS
% \item With FCI, good limit at CBS ==> exact energy
% \item But slow convergence with basis set because of divergence of the e-e interaction not well represented in atom centered basis set
% \item Exponential increase of number of Slater determinants
\item Cite papiers RS-DFT: there exists an hybrid scheme combining fast convergence wr to basis set (non divergent basis set) and short expansion in SCI (cite papier Ferté)
\item Question: does such a scheme provide better nodal quality ?
\item In RS-DFT we cannot optimize energy with $\mu$ , but in FNDMC
\item Factual stuffs: with optimal $\mu$, lower FNDMC energy than HF/KS/FCI
\begin{itemize}
\item less determinants $\Rightarrow$ large systems
\item only one parameter to optimize $\Rightarrow$ deterministic
\item $\Rightarrow$ reproducible
\end{itemize}
\item with the optimal $\mu$:
\begin{itemize}
\item Direct optimization of FNDMC with one parameter
\item Do we improve energy differences ?
\item system dependent
\item basis set dependent: $\mu \rightarrow \infty$ when $\mathcal{B}\rightarrow \text{CBS}$
\item large wave functions
\end{itemize}
\item Invariance with $m_s$
% \item Factual stuffs: with optimal $\mu$, lower FNDMC energy than HF/KS/FCI
% \begin{itemize}
% \item less determinants $\Rightarrow$ large systems
% \item only one parameter to optimize $\Rightarrow$ deterministic
% \item $\Rightarrow$ reproducible
% \end{itemize}
% \item with the optimal $\mu$:
% \begin{itemize}
% \item Direct optimization of FNDMC with one parameter
% \item Do we improve energy differences ?
% \item system dependent
% \item basis set dependent: $\mu \rightarrow \infty$ when $\mathcal{B}\rightarrow \text{CBS}$
% \item large wave functions
% \end{itemize}
\end{itemize}
\end{enumerate}
@ -940,15 +955,15 @@ Challenge 2019-gch0418) and from CALMIP (Toulouse) under allocation
\end{document}
% * Recouvrement avec Be
% * Tester sr-LDA avec H2O-DZ
% * Recouvrement avec Be : Optimization tous electrons
% impossible. Abandon. On va prendre H2O.
% * Manu doit faire des programmes pour des plots de ensite a 1 et 2
% corps le long des axes de liaison, et l'integrale de la densite a
% 2 corps a coalescence.
% 1 Manu calcule Be en cc-pvdz tous electrons: FCI -> NOs -> FCI ->
% qp edit -n 200
% 2 Manu calcule qp_cipsi_rsh avec mu = [ 1.e-6 , 0.25, 0.5, 1.0, 2.0, 5.0, 1e6 ]
% 3 Manu fait tourner es petits programmes
% 3 Manu fait tourner ses petits programmes
% 4 Manu envoie a toto un tar avec tous les ezfio
% 5 Toto optimise les coefs en presence e jastrow
% 6 Toto renvoie a manu psicoef