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Cosmological Evolution of Interacting Dark Energy Models with Mass Varying Neutrinos

Xiao-Jun Bi·Bo Feng·Hong Li·Xinmin Zhang
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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.

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Xiao-Jun Bi, Bo Feng, Hong Li, Xinmin Zhang. 2005-11-02. Cosmological Evolution of Interacting Dark Energy Models with Mass Varying Neutrinos. https://doi.org/10.1103/physrevd.72.123523

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