Constraints from observational data for a running cosmological constant and warm dark matter with curvature
General Relativity and Quantum Cosmology
2020-12-08 v2 Cosmology and Nongalactic Astrophysics
High Energy Physics - Theory
Abstract
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.
Keywords
Cite
@article{arxiv.2007.12636,
title = {Constraints from observational data for a running cosmological constant and warm dark matter with curvature},
author = {Jhonny A. Agudelo Ruiz and Júlio C. Fabris and Alan M. Velasquez-Toribio and Ilya L. Shapiro},
journal= {arXiv preprint arXiv:2007.12636},
year = {2020}
}
Comments
19 pages, 3 figures, 1 table. Two misprints corrected, accepted in "Gravitation and Cosmology"