% ****** Start of file apssamp.tex ****** % % This file is part of the APS files in the REVTeX 4.1 distribution. % Version 4.1r of REVTeX, August 2010 % % Copyright (c) 2009, 2010 The American Physical Society. % % See the REVTeX 4 README file for restrictions and more information. % % TeX'ing this file requires that you have AMS-LaTeX 2.0 installed % as well as the rest of the prerequisites for REVTeX 4.1 % % See the REVTeX 4 README file % It also requires running BibTeX. The commands are as follows: % % 1) latex apssamp.tex % 2) bibtex apssamp % 3) latex apssamp.tex % 4) latex apssamp.tex % \documentclass[% reprint, %superscriptaddress, %groupedaddress, %unsortedaddress, %runinaddress, %frontmatterverbose, %preprint, %showpacs,preprintnumbers, %nofootinbib, %nobibnotes, %bibnotes, amsmath,amssymb, aps, %pra, prb, %rmp, %prstab, %prstper, %floatfix, ]{revtex4-1} \usepackage{graphicx}% Include figure files \usepackage{physics}% brakets, etc.. \usepackage{dcolumn}% Align table columns on decimal point \usepackage{bm}% bold math \usepackage{multirow}% Added by H. Shin to plot multi-row table \usepackage{xcolor} \usepackage{amstext,amsmath,amssymb,amsfonts,braket} % Package Maths %\usepackage{hyperref}% add hypertext capabilities %\usepackage[mathlines]{lineno}% Enable numbering of text and display math %\linenumbers\relax % Commence numbering lines %\usepackage[showframe,%Uncomment any one of the following lines to test %%scale=0.7, marginratio={1:1, 2:3}, ignoreall,% default settings %%text={7in,10in},centering, %%margin=1.5in, %%total={6.5in,8.75in}, top=1.2in, left=0.9in, includefoot, %%height=10in,a5paper,hmargin={3cm,0.8in}, %]{geometry} \newcommand{\beq}{\begin{equation}} \newcommand{\eeq}{\end{equation}} \newcommand{\beqq}{\begin{equation*}} \newcommand{\eeqq}{\end{equation*}} \newcommand{\bal}{\begin{align}} \newcommand{\eal}{\end{align}} \newcommand{\bcen}{\begin{center}} \newcommand{\ecen}{\end{center}} \newcommand{\tsp}{\textsuperscript} \newcommand{\tsb}{\textsubscript} \begin{document} %\preprint{APS/123-QED} \title{Enabling high accuracy DMC calculations with Range Separated DFT nodes} %\\ breaks with \\ %\thanks{A footnote to the article title}% \author{Anouar Benali*}% \email{benali@anl.gov} \affiliation{Computational Sciences Division, Argonne National Laboratory, Argonne, IL 60439, United States} \author{Thomas Applencourt} \affiliation{Argonne Leadership Computing Facility, Argonne National Laboratory, Argonne, IL 60439, United States} \author{Pierre-Francois Loos} \author{Anthony Scemama*} \affiliation{Laboratoire de Chimie et Physique Quantiques, Universit\'e de Toulouse, CNRS, UPS, France} \author{Emanuel Giner*} \email{emmanuel.giner@lct.jussieu.fr} \affiliation{Laboratoire de Chimie Th\'eorique, Sorbonne Universit\'e and CNRS, F-75005 Paris, France} \date{\today}% It is always \today, today, % but any date may be explicitly specified \begin{abstract} %TODO Fixed Node approximation sucks. Best way to solve it is with multideterminants. sCI approach great but only for small systems. Large number of determinants comes from high energy determinants describing electron electron cusp in the same manner as 2 body Jastrow used in Diffusion Monte Carlo. Range Separated Density Functional Theory removes the cusp by using a DFT function (erf function) to describe the cusp and CIPSI for long range. Determinants are then selected without the electron electron cusp. \end{abstract} \pacs{Valid PACS appear here}% PACS, the Physics and Astronomy % Classification Scheme. %\keywords{Suggested keywords}%Use showkeys class option if keyword %display desired \maketitle %\tableofcontents \section{\label{sec:level1}Introduction} %TODO Single determinant diffusion Monte Carlo (SD-DMC) has proven to be very accurate at describing properties of a wide range of molecules and solids (citation). While closed-shell systems can reach accuracies of few kcal/mol for molecules and 0.05 to 0.1~eV for solids when compared to experimental data or coupled cluster calculations, a systematic accurate prediction of properties such as total energies and band/HOMO-LUMO gaps remains dependent on the nodes of the trial wavefunction; while DMC solves exactly the many-body Schr\"odinger equation, the fixed node approximation is the only practical way to maintain the fermionic behavior of the wavefunction and therefore is considered the \\ Using a CIPSI trial wavefunction in DMC allows a systematic improvement of the nodal surface for a large class of molecules (cite LCPQ papers) and solids(cite unpublished Diamond). However, while CIPSI allows for a very compact determinant expansion, we are still limited in practice to a few hundreds of atomic orbitals per system. Moreover, in many cases, even when it is possible to converge the CIPSI energy for a system, the size of determinant expansion is too large to be used in DMC as the wave function needs to be evaluated at every Monte Carlo step. While the DMC energy associated with the FCI wave function can be estimated by extrapolation, it is still desirable to find a strategy to reduce the size of the determinant expansions. %While the large number of determinants is often attributed to describing the electron-electron cusp, using a 2-body Jastrow often comes to achieving the same result at short range. \section{Short-range correlation} \newcommand{\psidet}{\Psi_{\text{CI}}} \newcommand{\psijas}{\exp(J)} The common practice in QMC calculations is to first compute a trial wave function expressed as a configuration interaction (CI) expansion $\psidet$. Then, the wave function is improved with a Jastrow factor $\psijas$ optimized in a variational Monte Carlo (VMC) framework. The role of the Jastrow factor is to take account explicitly of electron correlation and the simplest Jastrow factor is expressed as \begin{equation} J = \sum_{i