arXiv:0803.2637·v1·Astrophysics
Non-Gaussianity in three fluid curvaton model
Tuomas Multamaki🇫🇮 · Jani Sainio🇫🇮 · Iiro Vilja🇫🇮
Abstract
The generation of non-gaussianity is studied in a three fluid curvaton model. By utilizing second order perturbation theory we derive general formulae for the large scale temperature fluctuation and non-gaussianity parameter, , that includes the possibility of a non-adiabatic final state. In the adiabatic limit we recover previously known results. The results are applied to a three fluid curvaton model where the curvaton decays into radiation and matter. We find that the amount of non-gaussianity decreases as the final state of the system becomes more adiabatic and that the generated non-gaussianity in the scenario is small, .
Comments: 10 pages, 2 figures