Feynman rules and loop structure of Carrollian amplitudes

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Auteurs principaux: Liu, Wen-Bin, Long, Jiang, Ye, Xiao-Quan
Format: Preprint
Publié: 2024
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author Liu, Wen-Bin
Long, Jiang
Ye, Xiao-Quan
author_facet Liu, Wen-Bin
Long, Jiang
Ye, Xiao-Quan
contents In this paper, we derive the Carrollian amplitude in the framework of bulk reduction. The Carrollian amplitude is shown to relate to the scattering amplitude by a Fourier transform in this method. We propose Feynman rules to calculate the Carrollian amplitude where the Fourier transforms emerge as the integral representation of the external lines in the Carrollian space. Then we study the four-point Carrollian amplitude at loop level in massless $Φ^4$ theory. As a consequence of Poincaré invariance, the four-point Carrollian amplitude can be transformed to the amplitude that only depends on the cross ratio $z$ of the celestial sphere and a variable $χ$ invariant under translation. The four-point Carrollian amplitude is a polynomial of the two-point Carrollian amplitude whose argument is replaced with $χ$. The coefficients of the polynomial have branch cuts in the complex $z$ plane. We also show that the renormalized Carrollian amplitude obeys the Callan-Symanzik equation. Moreover, we initiate a generalized $Φ^4$ theory by designing the Feynman rules for more general Carrollian amplitude.
format Preprint
id arxiv_https___arxiv_org_abs_2402_04120
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Feynman rules and loop structure of Carrollian amplitudes
Liu, Wen-Bin
Long, Jiang
Ye, Xiao-Quan
High Energy Physics - Theory
In this paper, we derive the Carrollian amplitude in the framework of bulk reduction. The Carrollian amplitude is shown to relate to the scattering amplitude by a Fourier transform in this method. We propose Feynman rules to calculate the Carrollian amplitude where the Fourier transforms emerge as the integral representation of the external lines in the Carrollian space. Then we study the four-point Carrollian amplitude at loop level in massless $Φ^4$ theory. As a consequence of Poincaré invariance, the four-point Carrollian amplitude can be transformed to the amplitude that only depends on the cross ratio $z$ of the celestial sphere and a variable $χ$ invariant under translation. The four-point Carrollian amplitude is a polynomial of the two-point Carrollian amplitude whose argument is replaced with $χ$. The coefficients of the polynomial have branch cuts in the complex $z$ plane. We also show that the renormalized Carrollian amplitude obeys the Callan-Symanzik equation. Moreover, we initiate a generalized $Φ^4$ theory by designing the Feynman rules for more general Carrollian amplitude.
title Feynman rules and loop structure of Carrollian amplitudes
topic High Energy Physics - Theory
url https://arxiv.org/abs/2402.04120