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Stable Models of superacceleration

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arxiv astro-ph/0601517 v2 pith:C3JFYZFU submitted 2006-01-24 astro-ph

classification astro-ph
keywords modelsdarkenergyinstabilitysuperaccelerationabsentacausalapparent
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We discuss an instability in a large class of models where dark energy is coupled to matter. In these models the mass of the scalar field is much larger than the expansion rate of the Universe. We find models in which this instability is absent, and show that these models generically predict an apparent equation of state for dark energy smaller than -1, i.e., superacceleration. These models have no acausal behavior or ghosts.

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