Towards perturbative renormalization of $\phi^2(i\phi)^\varepsilon$ quantum field theory
Abstract
In a previous paper it was shown how to calculate the ground-state energy density and the -point Green's functions for the -symmetric quantum field theory defined by the Hamiltonian density in -dimensional Euclidean spacetime, where is a pseudoscalar field. In this earlier paper and were expressed as perturbation series in powers of and were calculated to first order in . (The parameter is a measure of the nonlinearity of the interaction rather than a coupling constant.) This paper extends these perturbative calculations to the Euclidean Lagrangian , which now includes renormalization counterterms that are linear and quadratic in the field . The parameter is a dimensionless coupling strength and is a scaling factor having dimensions of mass. Expressions are given for the one-, two, and three-point Green's functions, and the renormalized mass, to higher-order in powers of in dimensions (). Renormalization is performed perturbatively to second order in and the structure of the Green's functions is analyzed in the limit . A sum of the most divergent terms is performed to {\it all} orders in . Like the Cheng-Wu summation of leading logarithms in electrodynamics, it is found here that leading logarithmic divergences combine to become mildly algebraic in form. Future work that must be done to complete the perturbative renormalization procedure is discussed.
Cite
@article{arxiv.2103.07577,
title = {Towards perturbative renormalization of $\phi^2(i\phi)^\varepsilon$ quantum field theory},
author = {Alexander Felski and Carl M. Bender and S. P. Klevansky and Sarben Sarkar},
journal= {arXiv preprint arXiv:2103.07577},
year = {2021}
}
Comments
15 pages, 4 figures