Dark Energy: is it `just' Einstein's Cosmological Constant Lambda?
Ofer Lahav (UCL)

TL;DR
The paper reviews the role of the Cosmological Constant Lambda as Dark Energy, discussing its observational status, theoretical implications, current tensions, and future tests within the Lambda-CDM model.
Contribution
It provides a comprehensive overview of Lambda's significance in cosmology, highlighting current tensions and future prospects for understanding Dark Energy.
Findings
Lambda accounts for about 70% of the Universe's energy density.
Lambda-CDM model successfully explains many observations over 30 years.
Current tensions exist in measurements of the Hubble Constant and matter clumpiness.
Abstract
The Cosmological Constant Lambda, a concept introduced by Einstein in 1917, has been with us ever since in different variants and incarnations, including the broader concept of Dark Energy. Current observations are consistent with a value of Lambda corresponding to about present-epoch 70% of the critical density of the Universe. This is causing the speeding up (acceleration) of the expansion of the Universe over the past 6 billion years, a discovery recognised by the 2011 Nobel Prize in Physics. Coupled with the flatness of the Universe and the amount of 30% matter (5% baryonic and 25% Cold Dark Matter), this forms the so-called Lambda-CDM standard model, which has survived many observational tests over about 30 years. However, there are currently indications of inconsistencies (`tensions' ) within Lambda-CDM on different values of the Hubble Constant and the clumpiness factor. Also,…
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