New Exponential and Polynomial $\hat{I}¾$-attractors

Abstract

We introduce a new family of cosmological attractors with non-minimal coupling of gravity and non-canonical kinetic terms. In the Einstein frame, these models transform into a class of exponential and polynomial attractors with the spectral index $n_s$ spanning a broad range $1-2/N\le n_s<1-1/N$, and $r$ can decrease to zero in the limit $\hat{I}¾\to \infty$. This is sufficient to match any combination of Planck, BICEP/Keck, ACT, SPT, and DESI data. We present a supergravity implementation of these models.

19 pages, 6 figures, a reference added