THE COSMOLOGICAL STANDARD MODEL

The standard model of cosmology, also called the Lambda-CDM model, is the simplest theoretical framework able to provide a good description of all the observed cosmological phenomena with just 6 free parameters. In particular, the model predicts the existence and characteristics of the cosmic microwave background, baryon acoustic oscillations, large-scale structures in the distribution of galaxies, the abundance of light elements, and the accelerated expansion of the universe (due to the Lambda cosmological constant).

In the model, the validity of the cosmological principle is assumed (the universe is homogeneous and isotropic on large scales), as well as the general theory of relativity on cosmological distances and the standard model of elementary particles. The universe described by the model has its origin in the Big Bang, followed by a period of cosmic inflation in which the universe exponentially expands. The existence of non-baryonic dark matter that is cold (i.e. whose speed is much less than light’s in the epoch of matter-radiation equality) and with only gravitational interaction is also assumed to explain various gravitational phenomena observed in large-scale structures. These include the rotation curves of galaxies and the “gravitational lensing” effect of galactic masses.

Time Line of the Universe (© NASA/WMAP Science Team)
Map of the anisotropies of the cosmic microwave background seen by the ESA Planck satellite. (© Esa e Planck Collaboration)

Despite the great successes obtained, in particular with the measurements of the cosmic microwave background, some recent observations are not in complete agreement with the predictions of the Lambda-CDM model. These may indicate the need to reconsider the assumptions made or to modify the model. The most well known is the so-called “Hubble tension”. The determination of the Hubble constant (that measures the expansion speed ofthe universe) obtained by analysing the data of the cosmic microwave background in the context of the Lambda-CDM model is in partial disagreement with that obtained by measurements made using the stars and galaxies of the local universe. Various explanations have been put forward for this divergence, including the presence of “new physics” not described by the cosmological standard model.