Bounds on the Polymer Scale from Gamma Ray Bursts
arXiv:1704.08750 · doi:10.1103/PhysRevD.96.106021
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 , casting doubts on the possibility that the matter fields are quantized with the polymer representation we employed.
5 pages; Ver. 2: Two new references and some comments were added for more clarifications; Ver. 3: Based on referees' comments, some clarifications made in the text and the appendix, and a few citations added; Ver.4: final version matching PRD published article
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- Propagation of quantum gravity-modified gravitational waves on a classical FLRW spacetime
- Effective GUP-modified Raychaudhuri equation and black hole singularity: four models
- What do gravitational wave detectors say about polymer quantum effects?
- Casimir effect in polymer scalar field theory
- Quantum Groups and Polymer Quantum Mechanics
- Constraining the quantum gravity polymer scale using LIGO data