Matter non-conservation in the universe and dynamical dark energy

DOI10.1088/0264-9381/29/21/215002zbMath1266.83187arXiv1202.5097OpenAlexW3103231636MaRDI QIDQ4920154

Joan Solà, Harald Fritzsch

Publication date: 16 May 2013

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1202.5097

zbMATH Keywords

quantum field theoryexpanding universecurved spacetimedark mattervacuum energydark energyvacuum energy density

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Strong interaction, including quantum chromodynamics (81V05) Quantum field theory on curved space or space-time backgrounds (81T20) Methods of quantum field theory in general relativity and gravitational theory (83C47) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Astrophysical cosmology (85A40)

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About dark energy and dark matter in a three-dimensional quantum vacuum model ⋮ Scalar field theory description of the running vacuum model: the vacuumon ⋮ Dark Energy and the Time Dependence of Fundamental Particle Constants ⋮ Rényi Holographic dark energy models in multidimensional universe ⋮ Vacuum dynamics in the Universe versus a rigid Λ=const. ⋮ Accelerated expansion of the universe based on emergence of space and thermodynamics of the horizon ⋮ Brans–Dicke cosmology with a Λ-term: a possible solution to ΛCDM tensions* ⋮ Particle and entropy production in the running vacuum universe ⋮ The $\bar{\Lambda}{\rm CDM}$ cosmology: From inflation to dark energy through running Λ ⋮ The physical nature of the cosmological constant and the decoherence scale in a renormalization-group approach ⋮ Nonsingular decaying vacuum cosmology and entropy production

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