English

Phase dynamics and particle production in preheating

High Energy Physics - Phenomenology 2009-11-11 v3 Astrophysics

Abstract

We study a simple model of a massive inflaton field ϕ\phi coupled to another scalar filed χ\chi with interaction term g2ϕ2χ2g^2\phi^2\chi^2. We use the theory developed by Kofman {\em et al.} (Phys. Rev. D {\bf 56} (1997) 3258 [arXiv:hep-ph/9704452])for the first stage of preheating to give a full description of the dynamics of the χ\chi field modes, including the behaviour of the phase, in terms of the iteration of a simple family of circle maps. The parameters of this family of maps are a function of time when expansion of the universe is taken into account. With this more detailed description, we obtain a systematic study of the efficiency of particle production as a function of the inflaton field and coupling parameters, and we find that for g3×104g \lesssim 3 \times 10^{-4} the broad resonance ceases during the first stage of preheating.

Keywords

Cite

@article{arxiv.hep-ph/0502053,
  title  = {Phase dynamics and particle production in preheating},
  author = {T. Charters and A. Nunes and J. P. Mimoso},
  journal= {arXiv preprint arXiv:hep-ph/0502053},
  year   = {2009}
}

Comments

14 pages, 12 figures, accepted for publication in Phys. Rev. D. Correct Figure 9, results unchanged. Added references and corrected misprints/misspellings

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