Dynamics of phantom model with O(N) symmetry in loop quantum cosmology

Details Dynamics of phantom model with O(N) symmetry in loop quantum cosmology Dynamics of phantom model with O(N) symmetry in loop quantum cosmology

2010-06-04

arxiv.org/abs/1006.0811v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

9 pages, 3 figures

Scientific paper

Many astrophysical data show that the expansion of our universe is accelerating. In this paper, we study the model of phantom with O(N) symmetry in background of loop quantum cosmology(LQC). We investigate the phase-space stability of the corresponding autonomous system and find no stable node but only 2 saddle points in the field of real numbers. The dynamics is similar to the single-field phantom model in LQC[1]. The effect of O(N) symmetry just influence the detail of the universe's evolution. This is a sharp contrast with the result in general relativity, in which the dynamics of scalar fields models with O$(N)$ symmetry are quite different from the single-field models[2][3][4].

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