Derivation of a Vacuum Refractive Index in a Stringy Space-Time Foam Model
Abstract
It has been suggested that energetic photons propagating in vacuo should experience a non-trivial refractive index due to the foamy structure of space-time induced by quantum-gravitational fluctuations. The sensitivity of recent astrophysical observations, particularly of AGN Mk501 by the MAGIC Collaboration, approaches the Planck scale for a refractive index depending linearly on the photon energy. We present here a new derivation of this quantum-gravitational vacuum refraction index, based on a stringy analogue of the interaction of a photon with internal degrees of freedom in a conventional medium. We model the space-time foam as a gas of D-particles in the bulk space-time of a higher-dimensional cosmology where the observable Universe is a D3-brane. The interaction of an open string representing a photon with a D-particle stretches and excites the string, which subsequently decays and re-emits the photon with a time delay that increases linearly with the photon energy and is related to stringy uncertainty principles. We relate this derivation to other descriptions of the quantum-gravitational refractive index in vacuo.
Keywords
Cite
@article{arxiv.0804.3566,
title = {Derivation of a Vacuum Refractive Index in a Stringy Space-Time Foam Model},
author = {John Ellis and N. E. Mavromatos and D. V. Nanopoulos},
journal= {arXiv preprint arXiv:0804.3566},
year = {2008}
}
Comments
8 pages, 3 eps figures