# Bounds on the Polymer Scale from Gamma Ray Bursts

**Authors:** Yuri Bonder, Angel Garcia-Chung, Saeed Rastgoo

arXiv: 1704.08750 · 2017-12-01

## TL;DR

This paper investigates how polymer quantum representations affect electromagnetic field propagation and uses gamma ray burst data to set upper bounds on the polymer scale, challenging certain quantum gravity models.

## Contribution

It applies polymer quantization to the electromagnetic field and derives effective Hamiltonians, providing observational bounds on the polymer scale from gamma ray burst data.

## Key findings

- Polymer scale must be smaller than 4×10^{-35}
- Constraints challenge the viability of polymer quantization for matter fields
- Results link quantum gravity models to astrophysical observations

## Abstract

The polymer representations, which are partially motivated by loop quantum gravity, have been suggested as alternative schemes to quantize the matter fields. Here we apply a version of the polymer representations to the free electromagnetic field, in a reduced phase space setting, and derive the corresponding effective (i.e., semiclassical) Hamiltonian. We study the propagation of an electromagnetic pulse and we confront our theoretical results with gamma ray burst observations. This comparison reveals that the dimensionless polymer scale must be smaller than $4\times 10^{-35}$, casting doubts on the possibility that the matter fields are quantized with the polymer representation we employed.

## Full text

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## Figures

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## References

47 references — full list in the complete paper: https://tomesphere.com/paper/1704.08750/full.md

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Source: https://tomesphere.com/paper/1704.08750