English

Tachyonic Preheating in Plateau Inflation

Cosmology and Nongalactic Astrophysics 2022-01-24 v2 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology High Energy Physics - Theory

Abstract

Plateau inflation is an experimentally consistent framework in which the scale of inflation can be kept relatively low. Close to the edge of the plateau, scalar perturbations are subject to a strong tachyonic instability. Tachyonic preheating is realized when, after inflation, the oscillating inflaton repeatedly re-enters the plateau. We develop the analytic theory of this process and expand the linear approach by including backreaction between the coherent background and growing perturbations. For a family of plateau models, the analytic predictions are confronted with numerical estimates. Our analysis shows that the inflaton fragments in a fraction of an ee-fold in all examples supporting tachyonic preheating, generalizing the results of previous similar studies. In these scenarios, the scalar-to-tensor ratio is tiny, r<107r<10^{-7}.

Keywords

Cite

@article{arxiv.2108.10767,
  title  = {Tachyonic Preheating in Plateau Inflation},
  author = {Eemeli Tomberg and Hardi Veermäe},
  journal= {arXiv preprint arXiv:2108.10767},
  year   = {2022}
}

Comments

32 pages, 7 figures. v2: Updated to match published version. Added references

R2 v1 2026-06-24T05:22:56.870Z