Numerical study of the relativistic three-body quantization condition in the isotropic approximation
Abstract
We present numerical results showing how our recently proposed relativistic three-particle quantization condition can be used in practice. Using the isotropic (generalized -wave) approximation, and keeping only the leading terms in the effective range expansion, we show how the quantization condition can be solved numerically in a straightforward manner. In addition, we show how the integral equations that relate the intermediate three-particle infinite-volume scattering quantity, , to the physical scattering amplitude can be solved at and below threshold. We test our methods by reproducing known analytic results for the expansion of the threshold state, the volume dependence of three-particle bound-state energies, and the Bethe-Salpeter wavefunctions for these bound states. We also find that certain values of lead to unphysical finite-volume energies, and give a preliminary analysis of these artifacts.
Cite
@article{arxiv.1803.04169,
title = {Numerical study of the relativistic three-body quantization condition in the isotropic approximation},
author = {Raúl A. Briceño and Maxwell T. Hansen and Stephen R. Sharpe},
journal= {arXiv preprint arXiv:1803.04169},
year = {2018}
}
Comments
32 pages, 21 figures, JLAB-THY-18-2657, CERN-TH-2018-046; version 2: corrected typos, updated references, minor stylistic changes---consistent with published version