correction Fig 4

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Pierre-Francois Loos 2020-05-07 22:53:05 +02:00
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@ -184,16 +184,20 @@ that the deviation from linearity of the ensemble energy would be zero.}
\item \item
{Fig. 2: Why does the crossover point for the 1st excitation curves disappear for $L=8\pi$? } {Fig. 2: Why does the crossover point for the 1st excitation curves disappear for $L=8\pi$? }
\\ \\
\alert{It is clear from our derivations that the individual \alert{The legend of Fig.~2 was incorrect (the curves were mislabeled), but this has now been corrected.
correlation energies should vary with both the density {\it In the new Fig.~2 (which is now Fig.~4 in the revised manuscript), this crossover has disappeared and the discussion is much more fluid:
and} the ensemble weights. There is in principle no reason to expect the when the weight of a state increases, this state is stabilized while the two others increases in energy (as it should).
same variations for different ensembles and density regimes. The fact The discussion regarding this figure has been modified accordingly.}
that, for $L=8\pi$, electron correlation is strong and therefore the % \alert{It is clear from our derivations that the individual
density is more localized, is probably the reason for the disappearance %correlation energies should vary with both the density {\it
of the crossover point. We were not able to rationalize this observation %and} the ensemble weights. There is in principle no reason to expect the
further but we still mention in the revised manuscript that it is an %same variations for different ensembles and density regimes. The fact
illustration of the importance of both the density and the weights in %that, for $L=8\pi$, electron correlation is strong and therefore the
the evaluation of individual energies within an ensemble.} %density is more localized, is probably the reason for the disappearance
%of the crossover point. We were not able to rationalize this observation
%further but we still mention in the revised manuscript that it is an
%illustration of the importance of both the density and the weights in
%the evaluation of individual energies within an ensemble.}
\item \item
{Page 8: If the authors have evidence of behavior between $w=(0,0)$ and the equiensemble, instead of just these endpoints, that would be interesting to mention for the eDFT crowd. } {Page 8: If the authors have evidence of behavior between $w=(0,0)$ and the equiensemble, instead of just these endpoints, that would be interesting to mention for the eDFT crowd. }

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@ -867,7 +867,7 @@ Combining these, one can build the following three-state weight-dependent correl
%%% FIG 1 %%% %%% FIG 1 %%%
\begin{figure} \begin{figure}
\includegraphics[width=0.7\linewidth]{embedding} \includegraphics[width=0.7\linewidth]{fig1}
\caption{ \caption{
\label{fig:embedding} \label{fig:embedding}
\titou{Schematic view of the ``embedding'' scheme: the two-electron finite uniform electron gas (the impurity) is embedded in the infinite uniform electron gas (the bath). \titou{Schematic view of the ``embedding'' scheme: the two-electron finite uniform electron gas (the impurity) is embedded in the infinite uniform electron gas (the bath).
@ -952,7 +952,7 @@ For small $L$, the system is weakly correlated, while strong correlation effects
%%% FIG 1 %%% %%% FIG 1 %%%
\begin{figure} \begin{figure}
\includegraphics[width=\linewidth]{rho} \includegraphics[width=\linewidth]{fig2}
\caption{ \caption{
\titou{Ground-state one-electron density $\n{}{}(x)$ of 4-boxium (\ie, $N = 4$) for $L = \pi/32$ (left) and $L = 32\pi$ (right). \titou{Ground-state one-electron density $\n{}{}(x)$ of 4-boxium (\ie, $N = 4$) for $L = \pi/32$ (left) and $L = 32\pi$ (right).
In the weak correlation regime (small box length), the one-electron density is much more delocalized and uniform than in the strong correlation regime (large box length), where a Wigner crystal starts to appear. \cite{Rogers_2017,Rogers_2016}} In the weak correlation regime (small box length), the one-electron density is much more delocalized and uniform than in the strong correlation regime (large box length), where a Wigner crystal starts to appear. \cite{Rogers_2017,Rogers_2016}}
@ -996,7 +996,7 @@ equi-triensemble (or equal-weight state-averaged) limit where $\bw = (1/3,1/3)$.
%%% FIG 1 %%% %%% FIG 1 %%%
\begin{figure*} \begin{figure*}
\includegraphics[width=\linewidth]{EvsW_n5} \includegraphics[width=\linewidth]{fig3}
\caption{ \caption{
\label{fig:EvsW} \label{fig:EvsW}
Deviation from linearity of the weight-dependent KS-eLDA ensemble energy $\E{eLDA}{(\ew{1},\ew{2})}$ with (dashed lines) and without (solid lines) ghost-interaction correction (GIC) for 5-boxium (\ie, $\nEl = 5$) with a box of length $L = \pi/8$ (left), $L = \pi$ (center), and $L = 8\pi$ (right). Deviation from linearity of the weight-dependent KS-eLDA ensemble energy $\E{eLDA}{(\ew{1},\ew{2})}$ with (dashed lines) and without (solid lines) ghost-interaction correction (GIC) for 5-boxium (\ie, $\nEl = 5$) with a box of length $L = \pi/8$ (left), $L = \pi$ (center), and $L = 8\pi$ (right).
@ -1044,7 +1044,7 @@ Eqs.~\eqref{eq:min_with_HF_ener_fun} and \eqref{eq:WHF}].
%%% FIG 2 %%% %%% FIG 2 %%%
\begin{figure*} \begin{figure*}
\includegraphics[width=\linewidth]{EIvsW_n5} \includegraphics[width=\linewidth]{fig4}
\caption{ \caption{
\label{fig:EIvsW} \label{fig:EIvsW}
KS-eLDA individual energies, $\E{eLDA}{(0)}$ (black), $\E{eLDA}{(1)}$ (red), and $\E{eLDA}{(2)}$ (blue), as functions of the weights $\ew{1}$ (solid) and $\ew{2}$ (dashed) for 5-boxium (\ie, $\nEl = 5$) with a box of length $L = \pi/8$ (left), $L = \pi$ (center), and $L = 8\pi$ (right).} KS-eLDA individual energies, $\E{eLDA}{(0)}$ (black), $\E{eLDA}{(1)}$ (red), and $\E{eLDA}{(2)}$ (blue), as functions of the weights $\ew{1}$ (solid) and $\ew{2}$ (dashed) for 5-boxium (\ie, $\nEl = 5$) with a box of length $L = \pi/8$ (left), $L = \pi$ (center), and $L = 8\pi$ (right).}
@ -1058,14 +1058,18 @@ energies, which is in agreement with
the curvature of the GIC-eLDA ensemble energy discussed previously. Interestingly, the the curvature of the GIC-eLDA ensemble energy discussed previously. Interestingly, the
individual energies do not vary in the same way depending on the state individual energies do not vary in the same way depending on the state
considered and the value of the weights. considered and the value of the weights.
We see for example that, within the biensemble (\ie, $\ew{2}=0$), the energies of \titou{On one hand,} we see for example that, within the biensemble (\ie, $\ew{2}=0$), the energies of
the ground and first excited-state increase with respect to the the ground and \titou{second} excited-state increase with respect to the
first-excited-state weight $\ew{1}$, thus showing that, in this first-excited-state weight $\ew{1}$, thus showing that, in this
case, we case, we
``deteriorate'' these states by optimizing the orbitals for the ``deteriorate'' these states by optimizing the orbitals for the
ensemble, rather than for each state separately. The reverse actually occurs for the ground state in the triensemble ensemble, rather than for each state separately.
as $\ew{2}$ increases. The variations in the ensemble \titou{The singly excited state is, on the other hand, stabilize in the biensemble, which is reasonable as the weight associated with this state increases.
weights are essentially linear or quadratic. For the triensemble, as $\ew{2}$ increases, the energy of the ground state increases, while the energy of the first excited state remains stable with a slight increase at large $L$.
The second excited state is obviously stabilized by the increase of its weight in the ensemble.
These are all very sensible observations.}
The variations in the ensemble weights are essentially linear or quadratic.
\manurev{This can be rationalized as follows. As readily seen from \manurev{This can be rationalized as follows. As readily seen from
Eqs.~\eqref{eq:EI-eLDA} and \eqref{eq:ind_HF-like_ener}, the individual Eqs.~\eqref{eq:EI-eLDA} and \eqref{eq:ind_HF-like_ener}, the individual
HF-like energies do not depend explicitly on the weights, which means HF-like energies do not depend explicitly on the weights, which means
@ -1081,23 +1085,25 @@ weights $\bw$ [see Eqs.~\eqref{eq:ens1RDM},
\eqref{eq:ens_dens_from_ens_1RDM}, and \eqref{eq:ens_dens_from_ens_1RDM}, and
\eqref{eq:decomp_ens_correner_per_part}], the latter contributions will contain both linear and quadratic terms in \eqref{eq:decomp_ens_correner_per_part}], the latter contributions will contain both linear and quadratic terms in
$\bw$, as evidenced by Eq.~\eqref{eq:Taylor_exp_DDisc_term} [see the second term on the right-hand $\bw$, as evidenced by Eq.~\eqref{eq:Taylor_exp_DDisc_term} [see the second term on the right-hand
side].} In the biensemble, the weight dependence of the first side].}
excitation energy is reduced as the correlation increases. On the other hand, switching from a bi- to a triensemble !!! In the biensemble, the weight dependence of the first
excitation energy is \titou{increased?} as the correlation increases, \titou{while the weight dependence of the second excitation energy is reduced}.
On the other hand, switching from a bi- to a triensemble
systematically enhances the weight dependence, due to the lowering of the systematically enhances the weight dependence, due to the lowering of the
ground-state energy, as $\ew{2}$ increases. ground-state energy, as $\ew{2}$ increases.
The reverse is observed for the second excited state. The reverse is observed for the second excited state. !!! \titou{THIS PARAGRAPH MIGHT NEED MODIFICATIONS.}
\manurev{Finally, we notice that the crossover point of the \trashPFL{Finally, we notice that the crossover point of the
first-excited-state energies based on first-excited-state energies based on
bi- and triensemble calculations, respectively, disappears in the strong correlation bi- and triensemble calculations, respectively, disappears in the strong correlation
regime [see the right panel of Fig.~\ref{fig:EIvsW}], thus illustrating regime [see the right panel of Fig.~\ref{fig:EIvsW}], thus illustrating
the importance of (individual and ensemble) densities, in the importance of (individual and ensemble) densities, in
addition to the addition to the
weights, in the evaluation of individual energies within weights, in the evaluation of individual energies within
an ensemble. an ensemble.
} }
%%% FIG 3 %%% %%% FIG 3 %%%
\begin{figure} \begin{figure}
\includegraphics[width=\linewidth]{EvsL_5} \includegraphics[width=\linewidth]{fig5}
\caption{ \caption{
\label{fig:EvsL} \label{fig:EvsL}
Excitation energies (multiplied by $L^2$) associated with the single excitation $\Ex{}{(1)}$ (bottom) and double excitation $\Ex{}{(2)}$ (top) of 5-boxium for various methods and box lengths $L$. Excitation energies (multiplied by $L^2$) associated with the single excitation $\Ex{}{(1)}$ (bottom) and double excitation $\Ex{}{(2)}$ (top) of 5-boxium for various methods and box lengths $L$.
@ -1132,7 +1138,7 @@ This conclusion is verified for smaller and larger numbers of electrons
%%% FIG 4 %%% %%% FIG 4 %%%
\begin{figure*} \begin{figure*}
\includegraphics[width=\linewidth]{EvsN} \includegraphics[width=\linewidth]{fig6}
\caption{ \caption{
\label{fig:EvsN} \label{fig:EvsN}
Error with respect to FCI in single and double excitation energies for $\nEl$-boxium for various methods and electron numbers $\nEl$ at $L=\pi/8$ (left), $L=\pi$ (center), and $L=8\pi$ (right). Error with respect to FCI in single and double excitation energies for $\nEl$-boxium for various methods and electron numbers $\nEl$ at $L=\pi/8$ (left), $L=\pi$ (center), and $L=8\pi$ (right).
@ -1170,7 +1176,7 @@ electrons.
%%% FIG 5 %%% %%% FIG 5 %%%
\begin{figure*} \begin{figure*}
\includegraphics[width=\linewidth]{EvsL_DD} \includegraphics[width=\linewidth]{fig7}
\caption{ \caption{
\label{fig:EvsL_DD} \label{fig:EvsL_DD}
Error with respect to FCI (in \%) associated with the single excitation $\Ex{}{(1)}$ (bottom) and double excitation $\Ex{}{(2)}$ (top) as a function of the box length $L$ for 3-boxium (left), 5-boxium (center), and 7-boxium (right) at the KS-eLDA level with and without the contribution of the ensemble correlation derivative $\DD{c}{(I)}$. Error with respect to FCI (in \%) associated with the single excitation $\Ex{}{(1)}$ (bottom) and double excitation $\Ex{}{(2)}$ (top) as a function of the box length $L$ for 3-boxium (left), 5-boxium (center), and 7-boxium (right) at the KS-eLDA level with and without the contribution of the ensemble correlation derivative $\DD{c}{(I)}$.
@ -1227,7 +1233,7 @@ shown).
%%% FIG 6 %%% %%% FIG 6 %%%
\begin{figure} \begin{figure}
\includegraphics[width=\linewidth]{EvsN_DD} \includegraphics[width=\linewidth]{fig8}
\caption{ \caption{
\label{fig:EvsN_DD} \label{fig:EvsN_DD}
Error with respect to FCI in single and double excitation energies for $\nEl$-boxium (with a box length of $L=8\pi$) as a function of the number of electrons $\nEl$ at the KS-eLDA level with and without the contribution of the ensemble correlation derivative $\DD{c}{(I)}$. Error with respect to FCI in single and double excitation energies for $\nEl$-boxium (with a box length of $L=8\pi$) as a function of the number of electrons $\nEl$ at the KS-eLDA level with and without the contribution of the ensemble correlation derivative $\DD{c}{(I)}$.

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