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arXiv · gr-qc/0410096

Phantom Cosmology with Non-minimally Coupled Real Scalar Field

Abstract

We find that the expansion of the universe is accelerating by analyzing the recent observation data of type $\textsc{I}a$ supernova(SN-Ia) .It indicates that the equation of state of the dark energy might be smaller than -1,which leads to the introduction of phantom models featured by its negative kinetic energy to account for the regime of equation of state parameter $w<-1$.In this paper the possibility of using a non-minimally coupled real scalar field as phantom to realize the equation of state parameter $w<-1$ is discussed.The main equations which govern the evolution of the universe are obtained.Then we rewrite them with the observable quantities.

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BibTeXRIS

Zu-Yao Sun, You-Gen Shen. 2004-10-20. Phantom Cosmology with Non-minimally Coupled Real Scalar Field. https://doi.org/10.1007/s10714-005-0014-2

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