Constraints from observational data for a running cosmological constant
  and warm dark matter with curvature
  It is known than the inclusion of spatial curvature can modify the evolution
of matter perturbations and affect the Large Scale Structure (LSS) formation.
We quantify the effects of the non-zero space curvature in terms of LSS
formation for a cosmological model with a running vacuum energy density and a
warm dark matter component. The evolution of density perturbations and the
modified shape of its power spectrum are constructed and analyzed.
