Linear and non-linear perturbations in dark energy models
Nov, 2003Citations per year
Abstract: (arXiv)
I review the linear and second-order perturbation theory in dark energy models with explicit interaction to matter in view of applications to N-body simulations and non-linear phenomena. Several new or generalized results are obtained: the general equations for the linear perturbation growth: an analytical expression for the bias induced by a species-dependent interaction: the Yukawa correction to the gravitational potential due to dark energy interaction: the second-order perturbation equations in coupled dark energy and their Newtonian limit. I also show that a density-dependent effective dark energy mass arises if the dark energy coupling is varying.- 98.80.Cq
- dark energy
- perturbation: linear
- perturbation: nonlinear
- gravitation: potential
- correction: Yukawa
- field theory: scalar
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