Escher in the Sky
Renata Kallosh, Andrei Linde
TL;DR
The paper argues that inflationary predictions are governed not by the detailed inflaton potential but by the geometry of the moduli space, specifically a hyperbolic disk of radius √(3α). Through disk and half-plane formulations in supergravity, it shows how α-attractors yield universal predictions n_s ≈ 1 − 2/N and r ≈ 12α/N^2, with small α driving a plateau-like potential and robust observational consequences. It connects this cosmological framework to the SU(1,1) symmetry of superconformal theories, Escher-inspired geometric intuitions, and the FRW open-geometry analogy, providing concrete constructions via Kähler potentials and superpotentials that reproduce the attractor behavior across a broad class of models. The work highlights a geometry-driven path to consistent early-un universe physics, suggesting that future measurements of primordial gravitational waves could probe the underlying moduli-space geometry and its associated symmetries.
Abstract
The cosmological models called $α$-attractors provide an excellent fit to the latest observational data. Their predictions $n_{s} = 1-2/N$ and $r = 12α/N^{2}$ are very robust with respect to the modifications of the inflaton potential. An intriguing interpretation of $α$-attractors is based on a geometric moduli space with a boundary: a Poincare disk model of a hyperbolic geometry with the radius $\sqrt{3α}$, beautifully represented by the Escher's picture Circle Limit IV. In such models, the amplitude of the gravitational waves is proportional to the square of the radius of the Poincare disk.
