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Registro de acceso abierto On isotropic turbulence in the dark fluid universe

Autor :Brevik, Iver
Gorbunova, Olesya
Nojiri, Shin'ichi
Odintsov, Sergei D.
Fecha de publicación :26-abr-2011
Editor:Springer
Citación :European Physical Journal C - Particles and Fields 71 (4) : 1629 (2011
Resumen:As first part of this work, experimental information about the decay of isotropic turbulence in ordinary hydrodynamics, u^2(t) proportional to t^{-6/5}, is used as input in FRW equations in order to investigate how an initial fraction f of turbulent kinetic energy in the cosmic fluid influences the cosmological development in the late, quintessence/phantom, universe. First order perturbative theory to the first order in f is employed. It turns out that both in the Hubble factor, and in the energy density, the influence from the turbulence fades away at late times. The divergences in these quantities near the Big Rip behave essentially as in a non-turbulent fluid. However, for the scale factor, the turbulence modification turns out to diverge logarithmically. As second part of our work, we consider the full FRW equation in which the turbulent part of the dark energy is accounted for by a separate term. It is demonstrated that turbulence occurrence may change the future universe evolution due to dissipation of dark energy. For instance, phantom-dominated universe becomes asymptotically a de Sitter one in the future, thus avoiding the Big Rip singularity.
Descripción :The final publication is available at www.springerlink.com
Versión del editor:http://dx.doi.org/10.1140/epjc/s10052-011-1629-y
URI :http://hdl.handle.net/10261/37488
ISSN:1434-6044
E-ISSN:1434-6052
DOI:10.1140/epjc/s10052-011-1629-y
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