Decaying vacuum and evolution from early inflation to late acceleration

DOI10.1142/S0217732321501601zbMath1487.83134arXiv2103.15523MaRDI QIDQ5067264

Titus K. Mathew, N. Sarath

Publication date: 1 April 2022

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2103.15523

zbMATH Keywords

running vacuumprimordial perturbation wavelength

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Spectrum, resolvent (47A10) Geometrodynamics and the holographic principle (83E05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Perturbations in context of PDEs (35B20) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Traveling wave solutions (35C07)

Cites Work

• Variable cosmological constant as a Planck scale effect
• Cosmological constant -- the weight of the vacuum
• Holographic Ricci dark energy as running vacuum
• Dynamical cosmological term in modified gravity
• DYNAMICS OF DARK ENERGY
• Effective action of vacuum: the semiclassical approach
• Scalar field theory description of the running vacuum model: the vacuumon
• The $\bar{\Lambda}{\rm CDM}$ cosmology: From inflation to dark energy through running Λ
• The cosmological constant problem

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