English

Poly-instanton Inflation

High Energy Physics - Theory 2015-06-03 v1 Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology

Abstract

We propose a new inflationary scenario in type IIB Calabi-Yau compactifications, where the inflaton is a K\"ahler modulus parameterising the volume of an internal four-cycle. The inflaton potential is generated via poly-instanton corrections to the superpotential which give rise to a naturally flat direction due to their double exponential suppression. Given that the volume mode is kept stable during inflation, all the inflaton-dependent higher dimensional operators are suppressed. Moreover, string loop effects can be shown to be negligible throughout all the inflationary dynamics for natural values of the underlying parameters. The model is characterised by a reheating temperature of the order Trh106T_{\rm rh}\simeq 10^6 GeV which requires Ne54N_e \simeq 54 e-foldings of inflation. All the inflationary observables are compatible with current observations since the spectral index is ns0.96n_s \simeq 0.96, while the tensor-to-scalar ratio is r105r\simeq 10^{-5}. The volume of the Calabi-Yau is of order 10310^3 in string units, corresponding to an inflationary scale around 101510^{15} GeV

Keywords

Cite

@article{arxiv.1110.6182,
  title  = {Poly-instanton Inflation},
  author = {Michele Cicoli and Francisco G. Pedro and Gianmassimo Tasinato},
  journal= {arXiv preprint arXiv:1110.6182},
  year   = {2015}
}

Comments

20 pages, 4 figures

R2 v1 2026-06-21T19:27:11.385Z