2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/104443Finite expressions for the mean value of the stress tensor corresponding to a scalar field with a generalized dispersion relation in a Friedman--Robertson--Walker universe are obtained using adiabatic renormalization. Formally divergent integrals are evaluated by means of dimensional regularization. The renormalization procedure is shown to be equivalent to a redefinition of the cosmological constant and the Newton constant in the semiclassical Einstein equations.14 pages. Minor changes; version published in Physical Review DGeneral Relativity and Quantum CosmologyHigh Energy Physics - PhenomenologyHigh Energy Physics - TheoryRenormalized Stress Tensor for trans-Planckian Cosmologytext