Running vacuum cosmological models: linear scalar perturbations

DOI10.1088/1475-7516/2017/08/026OpenAlexW3098608419MaRDI QIDQ5021044

E. L. D. Perico, D. A. Tamayo

Publication date: 11 January 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1607.07825

zbMATH Keywords

cosmological perturbation theorydark energy theory

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (4)

Non-linear coupling in the dark sector as a running vacuum model ⋮ Perturbations in the interacting vacuum ⋮ Constraints from observational data for a running cosmological constant and warm dark matter with curvature ⋮ Particle and entropy production in the running vacuum universe

Uses Software

• GitHub
• CLASS

Cites Work

• On the growth of perturbations in interacting dark energy and dark matter fluids
• Cosmological model with interactions in the dark sector
• Variable cosmological constant as a Planck scale effect
• Running cosmological constant with observational tests
• Cosmological constant -- the weight of the vacuum
• THE ΛCDM GROWTH RATE OF STRUCTURE REVISITED
• The cosmological constant and dark energy
• COSMOLOGICAL PERTURBATIONS AND THE RUNNING COSMOLOGICAL CONSTANT MODEL
• Cosmic perturbations with running G and Λ
• THEORETICAL MODELS OF DARK ENERGY
• Decaying vacuum inflationary cosmologies: Searching for a complete scenario including curvature effects
• Production of primordial gravitational waves in a simple class of running vacuum cosmologies
• Dark energy: a quantum fossil from the inflationary universe?
• The cosmological constant problem
• The running of the cosmological and the Newton constants controlled by the cosmological event horizon
• Cosmic expansion and structure formation in running vacuum cosmologies
• CLASS

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