pith. sign in

arxiv: 1203.5316 · v1 · pith:HB7VNSUUnew · submitted 2012-03-23 · 🌌 astro-ph.CO · hep-ph· hep-th

Curvaton preheating revisited

classification 🌌 astro-ph.CO hep-phhep-th
keywords preheatingpycoolcurvatonnon-gaussianityprogramresultssimulationsthermalization
0
0 comments X
read the original abstract

We study the thermalization process in the self-interacting curvaton preheating scenario. We solve the evolution of the system with classical lattice simulations with a recently released symplectic PyCOOL program during the resonance and the early thermalization periods and compare the results to the inflaton preheating. After this we calculate the generated non-gaussianity with the $\Delta N$ formalism and the separate universe approximation by running a large number of simulations with slightly different initial values. The results indicate a high level of non-gaussianity. We also use this paper to showcase the various post-processing functions included with the PyCOOL program that is available from https://github.com/jtksai/PyCOOL .

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.