Reinterpretation of the Starobinsky model
Takehiko Asaka, Satoshi Iso, Hikaru Kawai, Kazunori Kohri, Toshifumi, Noumi, Takahiro Terada

TL;DR
This paper explains the peculiar form of the Starobinsky inflation model through extra-dimensional compactification, predicting observable inflationary parameters and suggesting quantum gravity effects at high energy scales.
Contribution
It offers a novel explanation for the Starobinsky model's action form based on extra dimensions, reducing the need for fine-tuning of higher-order terms.
Findings
Predicted spectral index and its runnings consistent with observations
Estimated tensor-to-scalar ratio within observable range
Proposed quantum gravity effects at high energy scale
Abstract
The Starobinsky model of inflation, consistent with Planck 2015, has a peculiar form of the action, which contains the leading Einstein term , the 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 is accepted to suppress the linear term , 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 GeV.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
