saving work: more Surjan and starting Hubbard MP

This commit is contained in:
Pierre-Francois Loos 2020-11-15 22:36:35 +01:00
parent de97e45b34
commit 59cc48bef0
9 changed files with 78 additions and 4 deletions

View File

@ -411,14 +411,88 @@ Even if there were still shaded areas in their analysis and that their classific
Recently, Mih\'alka \textit{et al.} studied the partitioning effect on the convergence properties of Rayleigh-Schr\"odinger perturbation theory by considering the MP and the EN partitioning as well as an alternative partitioning. \cite{Mihalka_2017a}
Taking as an example (in particular) the water molecule at equilibrium and at stretched geometries, they could estimate the radius of the convergence via a quadratic Pad\'e approximant and convert divergent perturbation expansions to convergent ones in some cases thanks to a judicious choice of the level shift parameter.
In a subsequent study by the same group, \cite{Mihalka_2017b} they use analytic continuation techniques to resum divergent series taking again as an example the water molecule in a stretched geometry.
In a subsequent study by the same group, \cite{Mihalka_2017b} they use analytic continuation techniques to resum divergent MP series taking again as an example the water molecule in a stretched geometry.
In a nutshell, their idea consists in calculating the energy of the system for several values of $\lambda$ for which the MP series is rapidly convergent, and to extrapolate the final energy to the physical system at $\lambda = 1$ via a polynomial- or Pad\'e-based fit.
However, the choice of the functional form of the fit remains a subtle task.
This technique was first generalized by using complex scaling parameters and applying analytic continuation by solving the Laplace equation, \cite{Surjan_2018} and then further improved thanks to Cauchy's integral formula
This technique was first generalized by using complex scaling parameters and applying analytic continuation by solving the Laplace equation, \cite{Surjan_2018} and then further improved thanks to Cauchy's integral formula \cite{Mihalka_2019}
\begin{equation}
\frac{1}{2\pi i} \oint \frac{E(z)}{z - a} = E(a)
\label{eq:Cauchy}
\frac{1}{2\pi i} \oint_{\gamma} \frac{E(z)}{z - a} = E(a).
\end{equation}
instead of the solution of the Laplace equation. \cite{Mihalka_2019}
Their method consists in refining self-consistently the values of $E(z)$ computed on a contour going through the physical point at $z = 1$ and encloses points of the ``trusted'' region (where the MP series is convergent). The shape of this contour is arbitrary but no singularities are allowed inside the contour to ensure $E(z)$ is analytic.
When the values of $E(z)$ on the so-called contour are converged, Cauchy's integrals formula \eqref{eq:Cauchy} is invoked to compute the values at $E(z=1)$ which corresponds to the final estimate of the FCI energy.
The authors illustrate this protocol on the dissociation curve of \ce{LiH} and the stretched water molecule showing encouraging results. \cite{Mihalka_2019}
%%% FIG 2 %%%
\begin{figure*}
\includegraphics[height=0.25\textwidth]{fig2a}
\hspace{0.05\textwidth}
\includegraphics[height=0.25\textwidth]{fig2b}
\hspace{0.05\textwidth}
\includegraphics[height=0.25\textwidth]{fig2c}
\caption{
Convergence of the RMP series as a function of the perturbation order $n$ energies for the Hubbard dimer at $U/t = 3.5$ (before the radius of convergence) and $4.5$ (after the radius of convergence).
The Riemann surfaces of the FCI energies are also represented for these two values of $U/t$.
\label{fig:RMP}}
\end{figure*}
Let us illustrate the behavior of the RMP and UMP series on the Hubbard dimer (see Fig.~\ref{fig:RMP}).
Within the RMP parition thecnique, we have
\begin{equation}
\label{eq:H_RMP}
\bH^\text{RMP} =
\begin{pmatrix}
-2t + U - \lambda U/2 & 0 & 0 & \lambda U/2 \\
0 & U - \lambda U/2 & \lambda U/2 & 0 \\
0 & \lambda U/2 & U - \lambda U/2 & 0 \\
\lambda U/2 & 0 & 0 & 2t + U - \lambda U/2 \\
\end{pmatrix},
\end{equation}
which yields the ground-state energy
\begin{equation}
\label{eq:E0MP}
E_0(\lambda) = U - \frac{\lambda U}{2} - \frac{1}{2} \sqrt{(4t)^2 + \lambda ^2 U^2}
\end{equation}
From this expression, it is easy to identify that the radius of convergence is defined by the exceptional points at $\lambda = \pm i 4t / U$ (which is similar to the FCI exceptional point).
Equation \eqref{eq:E0MP} can be Taylor expanded in terms of $\lambda$ to obtain the $n$th-order MP correction
\begin{equation}
E_0^{(n)} = U \delta_{0,n} - \frac{1}{2} \frac{U^n}{(4t)^{n-1}} \mqty( n/2 \\ 1/2)
\end{equation}
with
\begin{equation}
E_0(\lambda) = \sum_{n=0}^\infty E_0^{(n)} \lambda^n
\end{equation}
We illustrate this by plotting the energy expansions at orders of $\lambda$ just below and above the radius of convergence in Fig.~\ref{fig:RMP}.
\titou{T2 is going to add a discussion about this figure.}
At the UMP level now, we have
\begin{widetext}
\begin{equation}
\label{eq:H_UMP}
\bH^\text{UMP} =
\begin{pmatrix}
-2t^2 \lambda/U & 0 & 0 & +2t^2 \lambda/U \\
0 & U - 2t^2 \lambda/U & +2t^2\lambda/U & +2t \sqrt{U^2 - (2t)^2} \lambda/U \\
0 & +2t^2\lambda/U & U - 2t^2 \lambda/U & -2t \sqrt{U^2 - (2t)^2} \lambda/U \\
+2t^2 \lambda/U & +2t \sqrt{U^2 - (2t)^2} \lambda/U & -2t \sqrt{U^2 - (2t)^2} \lambda/U & 2U(1-\lambda) + 6t^2\lambda/U \\
\end{pmatrix},
\end{equation}
\end{widetext}
A closed-form expression for the ground-state energy can be obtained but it is cumbersome, so we eschew reporting its expression.
%%% FIG 3 %%%
\begin{figure*}
\includegraphics[height=0.25\textwidth]{fig3a}
\hspace{0.05\textwidth}
\includegraphics[height=0.25\textwidth]{fig3b}
\hspace{0.05\textwidth}
\includegraphics[height=0.25\textwidth]{fig3c}
\caption{
Convergence of the URMP series as a function of the perturbation order $n$ energies for the Hubbard dimer at $U/t = 3$ and $7$.
The Riemann surfaces of the FCI energies are also represented for these two values of $U/t$.
\label{fig:UMP}}
\end{figure*}
%==========================================%
\subsection{Insights from a two-state model}

BIN
Manuscript/fig1a.pdf Normal file

Binary file not shown.

BIN
Manuscript/fig1b.pdf Normal file

Binary file not shown.

BIN
Manuscript/fig2a.pdf Normal file

Binary file not shown.

BIN
Manuscript/fig2b.pdf Normal file

Binary file not shown.

BIN
Manuscript/fig2c.pdf Normal file

Binary file not shown.

BIN
Manuscript/fig3a.pdf Normal file

Binary file not shown.

BIN
Manuscript/fig3b.pdf Normal file

Binary file not shown.

BIN
Manuscript/fig3c.pdf Normal file

Binary file not shown.