# Multi-particle potentials from light-like Wilson lines in quark-gluon plasmas: a generalized relation of in-medium splitting rates to jet-quenching parameters $\hat q$

**Authors:** Peter Arnold

arXiv: 1901.05475 · 2025-06-23

## TL;DR

This paper generalizes the relation between in-medium splitting rates and jet-quenching parameters in quark-gluon plasmas, introducing multi-particle potentials derived from light-like Wilson lines to better understand medium effects on high-energy particles.

## Contribution

It introduces a method to determine N-body potentials from known jet-quenching parameters, extending the theoretical framework for in-medium QCD showering beyond previous two- and three-body formulations.

## Key findings

- N-body potentials can be inferred from jet-quenching parameters.
- For N > 3, potentials exhibit complex color structures.
- The approach simplifies calculations of overlap corrections in high-energy QCD processes.

## Abstract

A powerful historical insight about the theory of in-medium showering in QCD backgrounds was that splitting rates can be related to a parameter $\hat q$ that characterizes the rate of transverse-momentum kicks to a high-energy particle from the medium. Another powerful insight was that $\hat q$ can be defined (with caveats) even when the medium is strongly coupled, using long, narrow Wilson loops whose two long edges are light-like Wilson lines. The medium effects for the original calculations of in-medium splitting rates can be formulated in terms of 3-body imaginary-valued `potentials' that are defined with three long, light-like Wilson lines. Corrections due to overlap of two consecutive splittings can be calculated using similarly defined 4-body potentials. I give a simple argument for how such $N$-body potentials can be determined in the appropriate limit just from knowledge of the values of $\hat q$ for different color representations. For $N > 3$, the $N$-body potentials have non-trivial color structure, which will complicate calculations of overlap corrections outside of the large-$N_c$ or soft bremsstrahlung limits.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1901.05475/full.md

## References

26 references — full list in the complete paper: https://tomesphere.com/paper/1901.05475/full.md

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Source: https://tomesphere.com/paper/1901.05475