PREPRINT
9B11FD93-A7DB-4621-8B1D-401F6641BB3B

# Reissner-Nordstrom Expansion

Emil M. Prodanov, Rossen I. Ivanov, V. G. Gueorguiev
arXiv:hep-th/0703005

Submitted on 1 March 2007

## Abstract

We propose a classical mechanism for the cosmic expansion during the radiation-dominated era. This mechanism assumes that the Universe is a two-component gas. The first component is a gas of ultra-relativistic "normal" particles described by an equation of state of an ideal quantum gas of massless particles. The second component consist of "unusual" charged particles (namely, either with ultra-high charge or with ultra-high mass) that provide the important mechanism of expansion due to their interaction with the "normal" component of the gas. This interaction is described by the Reissner--Nordstr\"om metric purely geometrically -- the unusual'' particles are modeled as zero-dimensional naked singularities inside spheres of gravitational repulsion. The radius of a repulsive sphere is inversely proportional to the energy of an incoming particle or the temperature. The expansion mechanism is based on the inflating of the "unusual" particles (of charge $Q$) with the drop of the temperature -- this drives apart all neutral particles and particles of specific charge $q/m$ such that $sign\left(Q\right)q/m\ge -1$. The Reissner--Nordstr\"om expansion naturally ends at recombination. We discuss the range of model parameters within which the proposed expansion mechanism is consistent with the restrictions regarding quantum effects.

## Preprint

Comment: 9 pages, LaTeX

Subjects: High Energy Physics - Theory; Astrophysics; General Relativity and Quantum Cosmology