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تسجيل مستخدم جديدHidden past of dark energy cosmological models
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L. Fernandez-Jambrina
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In this paper we analyse the possibility of having homogeneous isotropic cosmological models with observers reaching $t=infty$ in finite proper time. It is shown that just observationally-suggested dark energy models with $win(-5/3,-1)$ show this feature and that they are endowed with an exotic curvature singularity. Furthermore, it is shown that non-accelerated observers in these models may experience a duration of the universe as short as desired by increasing their linear momentum. A subdivision of phantom models in two families according to this behavior is suggested.
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