English

Reinterpretation of the Starobinsky model

High Energy Physics - Theory 2016-12-13 v3 Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

The Starobinsky model of inflation, consistent with Planck 2015, has a peculiar form of the action, which contains the leading Einstein term RR, the R2R^2 term with a huge coefficient, and negligible higher-order terms. We propose an explanation of this form based on compactification of extra dimensions. Once tuning of order 10410^{-4} is accepted to suppress the linear term RR, we no longer have to suppress higher-oder terms, which give nontrivial corrections to the Starobinsky model. We show our predictions of the spectral index, its runnings, and the tensor-to-scalar ratio. Finally, we discuss a possibility that quantum gravity may appear at the scale Λ5×1015\Lambda \gtrsim 5 \times 10^{15} GeV.

Keywords

Cite

@article{arxiv.1507.04344,
  title  = {Reinterpretation of the Starobinsky model},
  author = {Takehiko Asaka and Satoshi Iso and Hikaru Kawai and Kazunori Kohri and Toshifumi Noumi and Takahiro Terada},
  journal= {arXiv preprint arXiv:1507.04344},
  year   = {2016}
}

Comments

13 pages, 2 figures; published version, references and discussion on the uncertainties of the predictions added

R2 v1 2026-06-22T10:12:37.376Z