English

Curvaton preheating revisited

Cosmology and Nongalactic Astrophysics 2015-06-04 v1 High Energy Physics - Phenomenology High Energy Physics - Theory

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 ΔN\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 .

Cite

@article{arxiv.1203.5316,
  title  = {Curvaton preheating revisited},
  author = {Jani Sainio},
  journal= {arXiv preprint arXiv:1203.5316},
  year   = {2015}
}

Comments

11 pages, 12 figures

R2 v1 2026-06-21T20:39:07.818Z