Old Inflation in String Theory
L. Pilo, A. Riotto, A. Zaffaroni

TL;DR
This paper introduces a string theory-based inflation model that avoids slow-roll conditions by utilizing warped compactifications and anti-D3-branes, providing a novel approach to early universe inflation.
Contribution
It presents a new string-inspired inflation scenario using warped geometries and anti-D3-branes, eliminating the need for a slow-roll inflaton potential.
Findings
Inflation driven by false vacuum with positive energy density.
Graceful exit achieved via anti-D3-branes migrating from ultraviolet to infrared.
Cosmological perturbations generated through the curvaton mechanism.
Abstract
We propose a stringy version of the old inflation scenario which does not require any slow-roll inflaton potential and is based on a specific example of string compatification with warped metric. Our set-up admits the presence of anti-D3-branes in the deep infrared region of the metric and a false vacuum state with positive vacuum energy density. The latter is responsible for the accelerated period of inflation. The false vacuum exists only if the number of anti-D3-branes is smaller than a critical number and the graceful exit from inflation is attained if a number of anti-D3-branes travels from the ultraviolet towards the infrared region. The cosmological curvature perturbation is generated through the curvaton mechanism.
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.
