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ACT-Inspired Kaehler-Based Inflationary Attractors (2507.02219v1)

Published 3 Jul 2025 in hep-ph, astro-ph.CO, and hep-th

Abstract: We develop a new class of cosmological attractors which are compatible with the recent ACT results. They are based on two types of fractional Kaehler potentials, K, for a gauge-singlet inflaton phi which reduce, along the inflationary path, to the form N/(1-phiqM)p with qM=1, 2 and 0.1< p<10. The combination of these K's with the chaotic potentials phin (where n=2, 4) within a non-linear sigma model leads to inflationary observables which are consistent with the current data and largely independent from qM and n. Endowing these K's with a shift symmetry we also offer a supergravity realization of our models introducing two chiral superfields and a monomial superpotential, linear with respect to the inflaton-accompanying field. The attainment of inflation with subplanckian inflaton values and the large values for the tensor-to-scalar ratio, which increases with N, are two additional attractive features of our proposal.

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