Abstract

Generic theories of quantum gravity often postulate that at some high energy/momentum scale there will be a fixed, minimal length. Such a minimal length can be phenomenologically investigated by modifying the standard Heisenberg Uncertainty relationship. This is generally done in practice by modifying the commutator between position and momentum operators, which in turn means modifying these operators. However, modifications such that the uncertainty relation changes lead to conflicts with observational data (gamma ray bursts). This arises in the form of a predicted minimal length energy scale that is above the Planck energy rather than below it. As a result there seems to be an implication that there is no minimal length scale in these generic theories. Meanwhile, modifying the operators such that the standard uncertainty relation retains the same form, leads to no such conflict with observational data. We show that it is this modification of the position and momentum operators that is the key determining factor in the existence (or not) of a minimal length scale. By focusing primarily on the role of these operators we also show that one can avoid the constraints from the observations of short gamma ray bursts, which in certain cases seem to push the minimal length scale above the Planck scale.

Highlights

  • Quantum gravity models often have the idea of a minimal distance at high energy/momentum scales [1]

  • Gamma ray bursts fall into two categories: (i) short gamma ray bursts which are thought to come from neutron star mergers or neutron star-black hole mergers and (ii) long gamma ray bursts which are thought to come from supernova

  • In this paper we present a minimal length scale model which does not lead to an energy dependent speed of light and avoids the constraints of the gamma ray bursts (GRB) observations

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Summary

Introduction

Quantum gravity models often have the idea of a minimal distance at high energy/momentum scales [1]. Gamma ray bursts are emissions of extremely high energy photons that generally are detected after traveling cosmological distances. In 2009 [7], the Fermi Gamma-Ray space telescope detected a short GRB (GRB090510) This observation allowed one to constrain the quantum gravity scale from 1.2 to 100 times the Planck scale depending on whether one made conservative or liberal assumptions (i.e. MQG ≥ 1.2MPl to MQG ≥ 100MPl). In this paper we present a minimal length scale model which does not lead to an energy dependent speed of light and avoids the constraints of the GRB observations. This can be accomplished with or without modifying the canonical commutation relationship

Modified energy-momentum relationship without photon dispersion
Minimal length via modified operators
Summary and Conclusions
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