Constraints from observational data for a running cosmological constant and warm dark matter with curvature

DOI10.1134/S0202289320040106zbMath1479.83048arXiv2007.12636OpenAlexW3044280886MaRDI QIDQ2246176

Jhonny A. Agudelo Ruiz, Alan M. Velasquez-Toribio, Ilya L. Shapiro, Júlio César Fabris

Publication date: 16 November 2021

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2007.12636

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Gravitational energy and conservation laws; groups of motions (83C40) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Dark matter and dark energy (83C56)

Related Items (1)

Analytical warm dark matter power spectrum on small scales

Cites Work

• Unnamed Item
• Variable cosmological constant as a Planck scale effect
• A new type of isotropic cosmological models without singularity
• The cosmological constant and dark energy
• COSMOLOGICAL PERTURBATIONS AND THE RUNNING COSMOLOGICAL CONSTANT MODEL
• RECONSTRUCTING DARK ENERGY
• Effective action of vacuum: the semiclassical approach
• Cosmic perturbations with running G and Λ
• Running vacuum cosmological models: linear scalar perturbations
• Nonlocal gravity. Conceptual aspects and cosmological predictions
• Theoretical foundations of the reduced relativistic gas in the cosmological perturbed context
• The cosmological constant problem
• SIMPLE COSMOLOGICAL MODEL WITH RELATIVISTIC GAS

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