Cosmological Evolution of Interacting Dark Energy Models with Mass Varying Neutrinos
High Energy Physics - Phenomenology
2007-05-23 v2 Astrophysics
High Energy Physics - Experiment
High Energy Physics - Theory
Abstract
In this paper we consider the cosmological implications of dark energy models with a coupled system of a dynamical scalar field (the quintessence) and the neutrinos. By detailed numerical calculations we study the various possibilities on the evolution and the fates of the universe in this class of models. Our results show that due to the interaction with quintessence, neutrinos could be dominant over the quintessence in the future universe, however would eventually decay away.
Keywords
Cite
@article{arxiv.hep-ph/0412002,
title = {Cosmological Evolution of Interacting Dark Energy Models with Mass Varying Neutrinos},
author = {Xiao-Jun Bi and Bo Feng and Hong Li and Xinmin Zhang},
journal= {arXiv preprint arXiv:hep-ph/0412002},
year = {2007}
}
Comments
One typographical error corrected, references updated and presentation improved