2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/199441We study the cosmological evolution of an induced gravity model with a self-interacting scalar field $σ$ and in the presence of matter and radiation. Such model leads to Einstein Gravity plus a cosmological constant as a stable attractor among homogeneous cosmologies and is therefore a viable dark-energy (DE) model for a wide range of scalar field initial conditions and values for its positive $γ$ coupling to the Ricci curvature $γσ^{2}R$.6 pages, 5 figures, 1 table: final version accepted for publication in PLBAstrophysicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theorytext