Analysis of scalar field cosmology with phase space deformations

Phase space deformations on scalar field cosmology are studied. The deformation is introduced by modifying the symplectic structure of the minisuperspace variables. The effects of the deformation are studied in the "C-frame" and the "NC-frame." In order to remove the ambiguities of working on different frames, a new principle is introduced. When we impose that both frames should be physically equivalent, we conclude that the only possibility for this model, is to have an effective cosmological constant Λ_eff≥0. Finally we bound the parameter space for θ and β.