Abstract

We present SUSY_LATTICE – a C++ program that can be used to simulate certain classes of supersymmetric Yang–Mills (SYM) theories, including the well known N=4 SYM in four dimensions, on a flat Euclidean space–time lattice. Discretization of SYM theories is an old problem in lattice field theory. It has resisted solution until recently when new ideas drawn from orbifold constructions and topological field theories have been brought to bear on the question. The result has been the creation of a new class of lattice gauge theories in which the lattice action is invariant under one or more supersymmetries. The resultant theories are local, free of doublers and also possess exact gauge-invariance. In principle they form the basis for a truly non-perturbative definition of the continuum SYM theories. In the continuum limit they reproduce versions of the SYM theories formulated in terms of twisted fields, which on a flat space–time is just a change of the field variables. In this paper, we briefly review these ideas and then go on to provide the details of the C++ code. We sketch the design of the code, with particular emphasis being placed on SYM theories with N=(2,2) in two dimensions and N=4 in three and four dimensions, making one-to-one comparisons between the essential components of the SYM theories and their corresponding counterparts appearing in the simulation code. The code may be used to compute several quantities associated with the SYM theories such as the Polyakov loop, mean energy, and the width of the scalar eigenvalue distributions. Program summaryProgram title: SUSY_LATTICECatalogue identifier: AELS_v1_0Program summary URL:http://cpc.cs.qub.ac.uk/summaries/AELS_v1_0.htmlProgram obtainable from: CPC Program Library, Queenʼs University, Belfast, N. IrelandLicensing provisions: Standard CPC license, http://cpc.cs.qub.ac.uk/licence/licence.htmlNo. of lines in distributed program, including test data, etc.: 9315No. of bytes in distributed program, including test data, etc.: 95 371Distribution format: tar.gzProgramming language: C++Computer: PCs and WorkstationsOperating system: Any, tested on Linux machinesClassification:: 11.6Nature of problem: To compute some of the observables of supersymmetric Yang–Mills theories such as supersymmetric action, Polyakov/Wilson loops, scalar eigenvalues and Pfaffian phases.Solution method: We use the Rational Hybrid Monte Carlo algorithm followed by a Leapfrog evolution and a Metropolis test. The input parameters of the model are read in from a parameter file.Restrictions: This code applies only to supersymmetric gauge theories with extended supersymmetry, which undergo the process of maximal twisting. (See Section 2 of the manuscript for details.)Running time: From a few minutes to several hours depending on the amount of statistics needed.

Highlights

  • The problem of formulating supersymmetric theories on lattices has a long history going back to the earliest days of lattice gauge theory

  • After initial efforts failed to produce useful supersymmetric lattice actions the topic languished for many years

  • The central problem is that naive discretizations of continuum supersymmetric theories break supersymmetry completely and radiative effects lead to a profusion of relevant supersymmetry breaking counterterms in the renormalized lattice action

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Summary

Introduction

The problem of formulating supersymmetric theories on lattices has a long history going back to the earliest days of lattice gauge theory. Having a lattice construction of the well known N = 4 SYM in four-dimensions is very advantageous from the point of view of exploring the connection between gauge theories and string/gravitational theories. Even without this connection to string theory, it is clearly of great importance to be able to give a non-perturbative formulation of a supersymmetric theory via a lattice path integral, in the same way that one can formally define QCD as a limit of lattice QCD as the lattice spacing goes to zero and the box size to infinity.

The method of topological twisting in SYM theories
Twisting the supersymmetries in d dimensions
A warm up example
Simulating the SYM theories
Numerical results
Eigenvalues of scalars
Restoration of supersymmetry
Conclusions
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