Dark energy: why is the expansion of the universe accelerating?

The enigma of {{strong|dark energy}} has fascinated astrophysicists for several decades. First observed with the discovery of a {{strong|cosmic acceleration}} in the expansion of {{strong|the universe}} at the end of the 20th century, this mysterious force challenges the classical knowledge of modern {{strong|cosmology}}. Constituting about 70% of the total content of the universe, as revealed … Read more

The H0 tension in modern cosmology

In brief: Accurate measurements and discrepancies in the Hubble constant: a challenge for modern cosmology The universe expansion is a reality observed for several decades, mathematically formalized by the Hubble-Lemaître law, which describes the linear relationship between the speed of galaxies moving away and their distance, with the Hubble constant (H0) as the proportionality factor. … Read more

The problem of the cosmological horizon

The cosmological horizon problem embodies one of the major challenges in modern cosmology, questioning the very foundations of our understanding of the observable universe. This conundrum raises a fascinating question: how can extremely distant regions of the universe, seemingly without any causal contact, exhibit such surprising homogeneity, particularly seen in the cosmic microwave background radiation? … Read more

The expansion of the universe: why and how

L'expansion de l'univers : pourquoi et comment

IN BRIEF Expansion of the Universe: phenomenon of galaxies moving away from each other. Observation by Edwin Hubble in 1929 on distance and redshift. Dynamic spaces: influence of gravity on space-time. Speed of expansion and its impact on cosmology. Origin of the Universe: about 13.8 billion years ago. Big Bang Theory and its implications for … Read more