Eleonora Di Valentino

TL;DR: In this paper, the authors present a thorough review of recent Hubble constant estimates and a summary of the proposed theoretical solutions, including early or dynamical dark energy, neutrino interactions, interacting cosmologies, primordial magnetic fields, and modified gravity.

TL;DR: In this article, the authors combine 23 Hubble constant measurements based on Cepheids-SN Ia, TRGB-SN II, Miras-SNIa, Masers, Tully Fisher, Surface Brightness Fluctuations, SN II, Time-delay Lensing, Standard Sirens and γ-ray Attenuation, obtaining the best optimistic H0 estimate, that is H0 = 72.7 ± 1.94 ± 0.75

TL;DR: In this paper, the authors investigated the possibility of phantom crossing in the dark energy sector and the solution for the Hubble tension between early and late universe observations using robust combinations of different cosmological observations, namely the Cosmic Microwave Background (CMB), local measurement of Hubble constant (H0), Baryon Acoustic Oscillation (BAO), and SnIa.

TL;DR: In this article, a global analysis of neutrino oscillation and nonoscillation data was performed, and the results of the analysis were shown to be consistent with the Planck results.

TL;DR: In this article, the neutrino mass limits were obtained by making use of the cosmic microwave background temperature fluctuation and polarization measurements, supernovae Ia luminosity distances, baryon acoustic oscillation observations and determinations of the growth rate parameter.