Vacuum dynamics in the Universe versus a rigid $\Lambda =$const

Abstract

In this year, in which we celebrate 100 years of the cosmological term, $\Lambda$, in Einstein's gravitational field equations, we are still facing the crucial question whether $\Lambda$ is truly a fundamental constant or a mildly evolving dynamical variable. After many theoretical attempts to understand the meaning of $\Lambda$, and in view of the enhanced accuracy of the cosmological observations, it seems now mandatory that this issue should be first settled empirically before further theoretical speculations on its ultimate nature. In this work, we summarize the situation of some of these studies. Devoted analyses made recently show that the $\Lambda =$const. hypothesis, despite being the simplest, may well not be the most favored one. The overall fit to the cosmological observables $SNIa+BAO+H(z)+LSS+CMB$ singles out the class RVM of the "running" vacuum models, in which $\Lambda =\Lambda (H)$ is an affine power-law function of the Hubble rate. It turns out that the performance of the RVM as compared to the "concordance" $\Lambda$CDM model (with $\Lambda =$const.) is much better. The evidence in support of the RVM may reach $\sim 4\sigma$ c.l., and is bolstered with Akaike and Bayesian criteria providing strong evidence in favor of the RVM option. We also address the implications of this framework on the tension between the CMB and local measurements of the current Hubble parameter.

Published in Int. J. Mod. Phys. A32 (2017) 1730014. arXiv admin note: text overlap with arXiv:1705.06723

References in corpus (15)

• The trouble with $H_0$
• Indications of a late-time interaction in the dark sector
• Dark energy: a quantum fossil from the inflationary Universe?
• Dynamical vacuum energy in the expanding Universe confronted with observations: a dedicated study
• Hubble expansion and structure formation in the "running FLRW model" of the cosmic evolution
• The $\bar{\Lambda }CDM$ cosmology: from inflation to dark energy through running $\Lambda$
• Determining $H_0$ with Bayesian hyper-parameters
• Vacuum models with a linear and a quadratic term in H: structure formation and number counts analysis
• Dynamical dark energy: scalar fields and running vacuum
• Nonsingular Decaying Vacuum Cosmology and Entropy Production
• Median statistics estimates of Hubble and Newton's Constant
• Effective growth of matter density fluctuations in the running LCDM and LXCDM models
• Fundamental constants and cosmic vacuum: the micro and macro connection
• Fundamental Constants in Physics and Their Time Variation
• Dark matter, dark energy and the time evolution of masses in the Universe

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