Abstract

In this article, we explicitly compute in momentum space the three and four-point correlation functions involving scalar and spinning operators in the free bosonic and the free fermionic theory in three dimensions. We also evaluate the five-point function of the scalar operator in the free bosonic theory. We discuss techniques which are more efficient than the usual PV reduction to evaluate one loop integrals. Our techniques can be easily generalised to momentum space correlators of complicated spinning operators and to higher point functions. The three dimensional fermionic theory has the interesting feature that the scalar operator overline{psi}psi is odd under parity. To account for this, we develop a parity odd basis which is useful to write correlation functions involving spinning operators and an odd number of overline{psi}psi operators. We further study higher spin (HS) equations in momentum space which are algebraic in nature and hence simpler than their position space counterparts. We use them to solve for three-point functions involving spinning operators without invoking conformal invariance. However, at the level of four-point functions, solving the HS equation requires additional constraints that come from conformal invariance and we could only verify that our explicit results solve the HS equation.

Highlights

  • Conformal field theory (CFT) plays a central role in theoretical physics

  • In particular we developed a basis for the transverse part of parity odd correlators

  • For four-point functions we could only verify that our explicit results solve the higher spin equation and not solve for them

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Summary

Introduction

Conformal field theory (CFT) plays a central role in theoretical physics. Three-point correlation functions in momentum space have been determined through conformal invariance in [5, 6, 10,11,12,13,14,15]. The absence of the analogue of conformal cross-ratios in momentum space makes the computation of four and higher point functions difficult. One of the reasons is its relation to Feynman graphs which are usually computed in momentum space It is significant for its applicability in the context of cosmology [22, 23, 30,31,32,33,34,35,36,37]. This is because descendants are related to primary operators by a simple multiplication of the momenta

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