We use a combination of Planck cosmic microwave background (CMB) anisotropy data and
non-CMB data that include Pantheon+ type Ia supernovae (SNIa), Hubble parameter [H (z)] …

We investigate a modified cosmological model aimed at addressing the Hubble tension,
considering revised dynamics in the late Universe. The model introduces a parameter c …

Cosmological data probe massive neutrinos via their effects on the geometry of the Universe
and the growth of structure, both of which are degenerate with the late-time expansion …

The fundamental constants at recombination can differ from their present-day values due to
degeneracies in cosmological parameters, raising the possibility of yet-undiscovered …

We study the performance of the spatially-flat dynamical dark energy (DE) $ w_0w_a $ CDM
parameterization, with redshift-dependent DE fluid equation of state parameter $ w (z) …

We propose a simple model that can alleviate the H 0 tension while remaining consistent
with big bang nucleosynthesis (BBN). It is based on a dark sector described by a standard …

A statistically significant detection of the diffuse supernova neutrino background (DSNB) is
around the corner. To this purpose, we assess the contribution to the DSNB of …

We study the behavior of the vacuum in Euclidean dynamical triangulations (EDT).
Algorithmic improvements and better lattice spacing determinations allow us to test the …

Conventional calibration of Baryon Acoustic Oscillations (BAO) data relies on estimation of
the sound horizon at drag epoch $ r_d $ from early universe observations by assuming a …

Dynamical system theory is a widely used technique in the analysis of cosmological models.
Within this framework, the equations describing the dynamics of a model are recast in terms …