comments for Hugh

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Pierre-Francois Loos 2020-11-30 22:43:30 +01:00
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@ -1268,29 +1268,20 @@ states which share the symmetry of the ground state,\cite{Goodson_2004} and are
(\subref{subfig:rmp_cp}) Exact critical points with $t=0$ occur on the negative real $\lambda$ axis (dashed). (\subref{subfig:rmp_cp}) Exact critical points with $t=0$ occur on the negative real $\lambda$ axis (dashed).
(\subref{subfig:rmp_cp_surf}) Modelling a finite basis using $t=0.1$ yields complex-conjugate EPs close to the (\subref{subfig:rmp_cp_surf}) Modelling a finite basis using $t=0.1$ yields complex-conjugate EPs close to the
real axis, giving a sharp avoided crossing on the real axis (solid). real axis, giving a sharp avoided crossing on the real axis (solid).
\titou{vertical axe label wrong in b.}
\label{fig:RMP_cp}} \label{fig:RMP_cp}}
\end{figure*} \end{figure*}
%------------------------------------------------------------------% %------------------------------------------------------------------%
% INTRODUCING THE MODEL % INTRODUCING THE MODEL
The simplified site basis of the Hubbard dimer makes explicilty modelling the ionisation continuum impossible. The simplified site basis of the Hubbard dimer makes explicilty modelling the ionisation continuum impossible.
Instead, we can use an asymmetric Hubbard dimer \cite{Carrascal_2015,Carrascal_2018} to consider one site as a ``ghost atom'' that acts as a Instead, we can use an asymmetric version of the Hubbard dimer \cite{Carrascal_2015,Carrascal_2018}
destination for ionised electrons. where we consider one of the sites as a ``ghost atom'' that acts as a
In this asymmetric model, we introduce a one-electron potential $-\epsilon$ on the left site to destination for ionised electrons being originally localised on the other site.
To mathematically model this scenario, in this asymmetric Hubbard dimer, we introduce a one-electron potential $-\epsilon$ on the left site to
represent the attraction between the electrons and the model ``atomic'' nucleus [see Eq.~\eqref{eq:H_FCI}], where we define $\epsilon > 0$. represent the attraction between the electrons and the model ``atomic'' nucleus [see Eq.~\eqref{eq:H_FCI}], where we define $\epsilon > 0$.
%The exact Hamiltonian [Eq.~\eqref{eq:H_FCI}] then becomes
%\begin{equation}
%\label{eq:H_FCI_Asymm}
%\bH =
%\begin{pmatrix}
% U-2\epsilon & -t & -t & 0 \\
% -t & -\epsilon & 0 & -t \\
% -t & 0 & -\epsilon & -t \\
% 0 & -t & -t & U \\
%\end{pmatrix}.
%\end{equation}
The reference Slater determinant for a doubly-occupied atom can be represented using the RHF The reference Slater determinant for a doubly-occupied atom can be represented using the RHF
orbitals [see Eq.~\eqref{eq:RHF_orbs}] with $\theta_{\alpha}^{\text{RHF}} = \theta_{\beta}^{\text{RHF}} = 0$. orbitals [see Eq.~\eqref{eq:RHF_orbs}] with $\theta_{\alpha}^{\text{RHF}} = \theta_{\beta}^{\text{RHF}} = 0$, which corresponds to strictly localise the two electrons on the left site.
%and energy %and energy
%\begin{equation} %\begin{equation}
% E_\text{HF}(0, 0) = \frac{1}{2} (2 U - 4 \epsilon). % E_\text{HF}(0, 0) = \frac{1}{2} (2 U - 4 \epsilon).
@ -1299,7 +1290,7 @@ With this representation, the parametrised RMP Hamiltonian becomes
\begin{widetext} \begin{widetext}
\begin{equation} \begin{equation}
\label{eq:H_RMP} \label{eq:H_RMP}
\bH_\text{RMP}\qty(\lambda) = \Tilde{\bH}_\text{RMP}\qty(\lambda) =
\begin{pmatrix} \begin{pmatrix}
2(U-\epsilon) - \lambda U & -\lambda t & -\lambda t & 0 \\ 2(U-\epsilon) - \lambda U & -\lambda t & -\lambda t & 0 \\
-\lambda t & (U-\epsilon) - \lambda U & 0 & -\lambda t \\ -\lambda t & (U-\epsilon) - \lambda U & 0 & -\lambda t \\
@ -1308,17 +1299,16 @@ With this representation, the parametrised RMP Hamiltonian becomes
\end{pmatrix}. \end{pmatrix}.
\end{equation} \end{equation}
\end{widetext} \end{widetext}
\titou{Shall we change the symbol $\bH_\text{RMP}\qty(\lambda)$ to avoid confusion? Maybe $\Tilde{\bH}_\text{RMP}\qty(\lambda)$?}
% DERIVING BEHAVIOUR OF THE CRITICAL SITE % DERIVING BEHAVIOUR OF THE CRITICAL SITE
For the ghost site to perfectly represent ionised electrons, the hopping term between the two sites must vanish with $t=0$. For the ghost site to perfectly represent ionised electrons, the hopping term between the two sites must vanish (\ie, $t=0$).
This limit corresponds to the dissociative regime in the asymmetric Hubbard dimer as discussed in Ref.~\onlinecite{Carrascal_2018}, This limit corresponds to the dissociative regime in the asymmetric Hubbard dimer as discussed in Ref.~\onlinecite{Carrascal_2018},
and the RMP energies become and the RMP energies become
\begin{subequations} \begin{subequations}
\begin{align} \begin{align}
E_{-} &= 2U - 2 \epsilon - U \lambda, E_{-} &= 2(U - \epsilon) - \lambda U,
\\ \\
E_{\text{S}} &= U - \epsilon - U \lambda, E_{\text{S}} &= (U - \epsilon) - \lambda U,
\\ \\
E_{+} &= U \lambda, E_{+} &= U \lambda,
\end{align} \end{align}
@ -1376,19 +1366,21 @@ set representations of the MP critical point.\cite{Sergeev_2006}
%------------------------------------------------------------------% %------------------------------------------------------------------%
% RELATIONSHIP BETWEEN QPT AND UMP % RELATIONSHIP BETWEEN QPT AND UMP
\titou{Returning to the symmetric Hubbard dimer?}
In Sec.~\ref{sec:spin_cont} we showed that the slow convergence of the UMP series for the strongly correlated In Sec.~\ref{sec:spin_cont} we showed that the slow convergence of the UMP series for the strongly correlated
Hubbard dimer was due to a complex-conjugate pair of EPs just outside the radius of convergence. Hubbard dimer was due to a complex-conjugate pair of EPs just outside the radius of convergence.
These EPs have positive real components and small imaginary components (Fig.~\ref{fig:UMP}), suggesting a potential These EPs have positive real components and small imaginary components (see Fig.~\ref{fig:UMP}), suggesting a potential
connection to MP critical points and QPTs (see Sec.~\ref{sec:MP_critical_point}). connection to MP critical points and QPTs (see Sec.~\ref{sec:MP_critical_point}).
For $\lambda>1$, the HF potential becomes an attractive component in Stillinger's For $\lambda>1$, the HF potential becomes an attractive component in Stillinger's
Hamiltonian displayed in Eq.~\eqref{eq:HamiltonianStillinger}, while the explicit electron-electron interaction Hamiltonian displayed in Eq.~\eqref{eq:HamiltonianStillinger}, while the explicit electron-electron interaction
becomes increasingly repulsive. becomes increasingly repulsive.
Critical points along the positive real $\lambda$ axis for closed-shell molecules then represent \titou{Critical points along the positive real $\lambda$ axis for closed-shell molecules then represent
points where the two-electron repulsion overcomes the attractive HF potential and an electron points where the two-electron repulsion overcomes the attractive HF potential and an electron
are successively expelled from the molecule.\cite{Sergeev_2006} are successively expelled from the molecule.\cite{Sergeev_2006}}
\titou{T2: I'd like to discuss that with you.}
Symmetry-breaking in the UMP reference creates different HF potentials for the spin-up and spin-down electrons. Symmetry-breaking in the UMP reference creates different HF potentials for the spin-up and spin-down electrons.
Consider the reference UHF solution where the spin-up and spin-down electrons are localised on the left and Consider one of the two reference UHF solutions where the spin-up and spin-down electrons are localised on the left and
right sites respectively. right sites respectively.
The spin-up HF potential will then be a repulsive interaction from the spin-down electron The spin-up HF potential will then be a repulsive interaction from the spin-down electron
density that is centred around the right site (and vice-versa). density that is centred around the right site (and vice-versa).
@ -1396,9 +1388,10 @@ As $\lambda$ becomes greater than 1 and the HF potentials become attractive, the
driving force for the electrons to swap sites. driving force for the electrons to swap sites.
This swapping process can also be represented as a double excitation, and thus an avoided crossing will occur This swapping process can also be represented as a double excitation, and thus an avoided crossing will occur
for $\lambda \geq 1$ (Fig.~\ref{subfig:ump_cp}). for $\lambda \geq 1$ (Fig.~\ref{subfig:ump_cp}).
Note that, although this appears to be an avoided crossing between the ground and first-excited state, \titou{Note that, although this appears to be an avoided crossing between the ground and first-excited state,
the earlier excited-state avoided crossing means that the first-excited state qualitatively the earlier excited-state avoided crossing means that the first-excited state qualitatively
represents the double excitation for $\lambda > 0.5.$ represents the double excitation for $\lambda > 0.5.$}
\titou{T2: I find it hard to understand. I'd like to discuss this as well.}
% SHARPNESS AND QPT % SHARPNESS AND QPT
The ``sharpness'' of the avoided crossing is controlled by the correlation strength $U/t$. The ``sharpness'' of the avoided crossing is controlled by the correlation strength $U/t$.
@ -1408,12 +1401,15 @@ This delocalisation dampens the electron swapping process and leads to a ``shall
that corresponds to EPs with non-zero imaginary components (solid lines in Fig.~\ref{subfig:ump_cp}). that corresponds to EPs with non-zero imaginary components (solid lines in Fig.~\ref{subfig:ump_cp}).
As $U/t$ becomes larger, the HF potentials become stronger and the on-site repulsion dominates the hopping As $U/t$ becomes larger, the HF potentials become stronger and the on-site repulsion dominates the hopping
term to make electron delocalisation less favourable. term to make electron delocalisation less favourable.
\titou{In other words, the electron localises on each site forming a so-called Wigner crystal.
T2: is it worth saying again?}
These effects create a stronger driving force for the electrons to swap sites until eventually this swapping These effects create a stronger driving force for the electrons to swap sites until eventually this swapping
occurs exactly at $\lambda = 1$. occurs exactly at $\lambda = 1$.
In this limit, the ground-state EPs approach the real axis (Fig.~\ref{subfig:ump_ep_to_cp}) and the avoided In this limit, the ground-state EPs approach the real axis (Fig.~\ref{subfig:ump_ep_to_cp}) and the avoided
crossing creates a gradient discontinuity in the ground-state energy (dashed lines in Fig.~\ref{subfig:ump_cp}). crossing creates a gradient discontinuity in the ground-state energy (dashed lines in Fig.~\ref{subfig:ump_cp}).
We therefore find that, in the strong correlation limit, the symmetry-broken ground-state EP becomes We therefore find that, in the strong correlation limit, the symmetry-broken ground-state EP becomes
a new type of MP critical and represents a QPT in the perturbation approximation. a new type of MP critical point \titou{and represents a QPT in the perturbation approximation}.
\titou{T2: what do you mean by this?}
Furthermore, this argument explains why the dominant UMP singularity lies so close, but always outside, the Furthermore, this argument explains why the dominant UMP singularity lies so close, but always outside, the
radius of convergence (see Fig.~\ref{fig:RadConv}). radius of convergence (see Fig.~\ref{fig:RadConv}).