Abstract

A systematization for the manipulations and calculations involving divergent (or not) Feynman integrals, typical of the one loop perturbative solutions of Quantum Field Theory, is proposed. A previous work on the same issue is generalized to treat theories and models having different species of massive fields. An improvement on the strategy is adopted so that no regularization needs to be used. The final results produced, however, can be converted into the ones of reasonable regularizations, especially those belonging to the dimensional regularization (in situations where the method applies). Through an adequate interpretation of the Feynman rules and a convenient representation for involved propagators, the finite and divergent parts are separated before the introduction of the integration in the loop momentum. Only the finite integrals obtained are in fact integrated. The divergent content of the amplitudes are written as a combination of standard mathematical object which are never really integrated. Only very general scale properties of such objects are used. The finite parts, on the other hand, are written in terms of basic functions conveniently introduced. The scale properties of such functions relate them to a well defined way to the basic divergent objects providing simple and transparent connection between both parts in the assintotic regime. All the arbitrariness involved in this type of calculations are preserved in the intermediary steps allowing the identification of universal properties for the divergent integrals, which are required for the maintenance of fundamental symmetries like translational invariance and scale independence in the perturbative amplitudes. Once these consistency relations are imposed no other symmetry is violated in perturbative calculations neither ambiguous terms survive at any theory or model formulated at any space-time dimension including nonrenormalizable cases. Representative examples of perturbative amplitudes involving different species of massive fermions are considered as examples. The referred amplitudes are calculated in detail within the context of the presented strategy (and systematization) and their relations among other Green functions are explicitly verified. At the end a generalization for the finite functions is presented.

Highlights

  • All the arbitrariness involved in this type of calculations are preserved in the intermediary steps allowing the identification of universal properties for the divergent integrals, which are required for the maintenance of fundamental symmetries like translational invariance and scale independence in the perturbative amplitudes

  • Given the fact that exact solutions for Quantum Field Theories (QFT) are rarely possible, almost all knowledge constructed through this formalism about the phenomenology of fundamental interacting particles has been obtained within the context of perturbative techniques

  • When we find a combination of divergent Feynman integrals in a certain step of the calculation of a perturbative amplitude, in order to give an additional step we have to specify the prescription we will adopt to handle the mathematical indefinitions involved

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Summary

Introduction

Given the fact that exact solutions for Quantum Field Theories (QFT) are rarely possible, almost all knowledge constructed through this formalism about the phenomenology of fundamental interacting particles has been obtained within the context of perturbative techniques. We would like to make the calculations preserving all the possible choices for the arbitrariness involved like those related to the choice of routings for the internal momenta and for the common scale for the finite and divergent parts. To complete such adequate calculational strategy it would be desirable to get a systematization for the finite parts of the amplitudes in a way that the mathematical expressions become simple allowing the required analysis and algebraic operations related to the renormalization procedures, among others. A generalization for the finite functions and their useful properties are presented in the Section 9 and, in the Section 10 we present our final remarks and conclusions

Basic One-Loop Feynman Integrals
N 1 k2
N 1 k2 2
Basic Structure Functions for the Finite Parts
Basic Two-Point Structure Functions
Basic Three-Point Structure Functions
Basic Four-Point Structure Functions
Manipulations and Calculations of the One-Loop Feynman Integrals
One-point Feynman Integrals
Two-Point Feynman Integrals
A2 2 2
A2 A3k k
A2 A3 k2 2 6
Four-Point Feynman Integrals
Physical Amplitudes
One-Point Functions
Two-Point Function
Iquad p p P P
Three-Point Functions
The Four-Vector Four-Point Function
Relations among Green Functions
Ambiguities and Symmetry relations
Generalizations of the Finite Functions and Their Relationship
10. Conclusions

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