Finite size spectrum of SU(N) principal chiral field from discrete Hirota dynamics

Using recently proposed method of discrete Hirota dynamics for integrable (1+1)D quantum field theories on a finite space circle of length L we derive and test numerically a finite system of nonlinear integral equations for the exact spectrum of energies of SU(N)×SU(N) principal chiral field model a...

Full description

Bibliographic Details
Main Authors: Vladimir Kazakov, Sébastien Leurent
Format: Article
Language:English
Published: Elsevier 2016-01-01
Series:Nuclear Physics B
Online Access:http://www.sciencedirect.com/science/article/pii/S0550321315003879
id doaj-ed79d96746b94343b9384db4b72f135f
record_format Article
spelling doaj-ed79d96746b94343b9384db4b72f135f2020-11-25T00:59:06ZengElsevierNuclear Physics B0550-32131873-15622016-01-01902C35438610.1016/j.nuclphysb.2015.11.012Finite size spectrum of SU(N) principal chiral field from discrete Hirota dynamicsVladimir Kazakov0Sébastien Leurent1Ecole Normale Superieure, LPT, 75231 Paris Cedex-5, FranceEcole Normale Superieure, LPT, 75231 Paris Cedex-5, FranceUsing recently proposed method of discrete Hirota dynamics for integrable (1+1)D quantum field theories on a finite space circle of length L we derive and test numerically a finite system of nonlinear integral equations for the exact spectrum of energies of SU(N)×SU(N) principal chiral field model as functions of mL, where m is the mass scale. We propose a determinant solution of the underlying Y-system, or Hirota equation, in terms of Wronskian determinants of N×N matrices parameterized by N−1 functions of the spectral parameter θ with the known analytic properties at finite L. Although the method works in principle for any state, the explicit equations are written for states in the U(1) sector only. For N>2, we encounter and clarify a few subtleties in these equations related to the presence of bound states, absent in the previously considered N=2 case. As a demonstration of efficiency of our method, we solve these equations numerically for a few low-lying states at N=3 in a wide range of mL.http://www.sciencedirect.com/science/article/pii/S0550321315003879
collection DOAJ
language English
format Article
sources DOAJ
author Vladimir Kazakov
Sébastien Leurent
spellingShingle Vladimir Kazakov
Sébastien Leurent
Finite size spectrum of SU(N) principal chiral field from discrete Hirota dynamics
Nuclear Physics B
author_facet Vladimir Kazakov
Sébastien Leurent
author_sort Vladimir Kazakov
title Finite size spectrum of SU(N) principal chiral field from discrete Hirota dynamics
title_short Finite size spectrum of SU(N) principal chiral field from discrete Hirota dynamics
title_full Finite size spectrum of SU(N) principal chiral field from discrete Hirota dynamics
title_fullStr Finite size spectrum of SU(N) principal chiral field from discrete Hirota dynamics
title_full_unstemmed Finite size spectrum of SU(N) principal chiral field from discrete Hirota dynamics
title_sort finite size spectrum of su(n) principal chiral field from discrete hirota dynamics
publisher Elsevier
series Nuclear Physics B
issn 0550-3213
1873-1562
publishDate 2016-01-01
description Using recently proposed method of discrete Hirota dynamics for integrable (1+1)D quantum field theories on a finite space circle of length L we derive and test numerically a finite system of nonlinear integral equations for the exact spectrum of energies of SU(N)×SU(N) principal chiral field model as functions of mL, where m is the mass scale. We propose a determinant solution of the underlying Y-system, or Hirota equation, in terms of Wronskian determinants of N×N matrices parameterized by N−1 functions of the spectral parameter θ with the known analytic properties at finite L. Although the method works in principle for any state, the explicit equations are written for states in the U(1) sector only. For N>2, we encounter and clarify a few subtleties in these equations related to the presence of bound states, absent in the previously considered N=2 case. As a demonstration of efficiency of our method, we solve these equations numerically for a few low-lying states at N=3 in a wide range of mL.
url http://www.sciencedirect.com/science/article/pii/S0550321315003879
work_keys_str_mv AT vladimirkazakov finitesizespectrumofsunprincipalchiralfieldfromdiscretehirotadynamics
AT sebastienleurent finitesizespectrumofsunprincipalchiralfieldfromdiscretehirotadynamics
_version_ 1725218929269276672