Curvature and isocurvature perturbations in a three-fluid model of curvaton decay

Details Curvature and isocurvature perturbations in a three-fluid model of curvaton decay Curvature and isocurvature perturbations in a three-fluid model of curvaton decay

2003-11-25

arxiv.org/abs/astro-ph/0311562v2

Phys.Rev. D69 (2004) 063513

Astronomy and Astrophysics

Astrophysics

15 pages, 8 figures, latex with revtex; v2: comment added on spectral tilt, to appear in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.69.063513

We study the evolution of the cosmological perturbations after inflation in curvaton models where the non-relativistic curvaton decays into both radiation and a cold dark matter component. We calculate the primordial curvature and correlated isocurvature perturbations inherited by the radiation and cold dark matter after the curvaton has decayed. We give the transfer coefficient in terms of the initial curvaton density relative to the curvaton decay rate.

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