In the realm of the Hubble tension—a review of solutions
The simplest ΛCDM model provides a good fit to a large span of cosmological data but
harbors large areas of phenomenology and ignorance. With the improvement of the number …
harbors large areas of phenomenology and ignorance. With the improvement of the number …
Finite-time cosmological singularities and the possible fate of the Universe
Singularities in any physical theory are either remarkable indicators of the unknown
underlying fundamental theory, or indicate a change in the description of the physical reality …
underlying fundamental theory, or indicate a change in the description of the physical reality …
On the evolution of the Hubble constant with the SNe Ia pantheon sample and baryon acoustic oscillations: a feasibility study for GRB-cosmology in 2030
MG Dainotti, B De Simone, T Schiavone, G Montani… - Galaxies, 2022 - mdpi.com
The difference from 4 to 6 σ in the Hubble constant (H 0) between the values observed with
the local (Cepheids and Supernovae Ia, SNe Ia) and the high-z probes (Cosmic Microwave …
the local (Cepheids and Supernovae Ia, SNe Ia) and the high-z probes (Cosmic Microwave …
Eppur è piatto? The cosmic chronometers take on spatial curvature and cosmic concordance
The question of whether cosmic microwave background (CMB) temperature and polarization
data from Planck favor a spatially closed universe with curvature parameter Ω K< 0 has been …
data from Planck favor a spatially closed universe with curvature parameter Ω K< 0 has been …
Testing general relativity in cosmology
M Ishak - Living Reviews in Relativity, 2019 - Springer
We review recent developments and results in testing general relativity (GR) at cosmological
scales. The subject has witnessed rapid growth during the last two decades with the aim of …
scales. The subject has witnessed rapid growth during the last two decades with the aim of …
Modified cosmology from extended entropy with varying exponent
We present a modified cosmological scenario that arises from the application of non-
extensive thermodynamics with varying exponent. We extract the modified Friedmann …
extensive thermodynamics with varying exponent. We extract the modified Friedmann …
Implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions
We perform a comprehensive analysis of the most common early-and late-universe
solutions to the H 0, Ly-α, and S 8 discrepancies. When considered on their own, massive …
solutions to the H 0, Ly-α, and S 8 discrepancies. When considered on their own, massive …
Scalar induced gravitational waves from primordial black hole Poisson fluctuations in f (R) gravity
The gravitational potential of a gas of initially randomly distributed primordial black holes
(PBH) can induce a stochastic gravitational-wave (GW) background through second-order …
(PBH) can induce a stochastic gravitational-wave (GW) background through second-order …
[HTML][HTML] Cosmology in f (R, Lm) gravity
In this letter, we investigate the cosmic expansion scenario of the universe in the framework
of f (R, L m) gravity theory. We consider a non-linear f (R, L m) model, specifically, f (R, L m) …
of f (R, L m) gravity theory. We consider a non-linear f (R, L m) model, specifically, f (R, L m) …
Structure formation in f (T) gravity and a solution for H0 tension
RC Nunes - Journal of Cosmology and Astroparticle Physics, 2018 - iopscience.iop.org
We investigate the evolution of scalar perturbations in f (T) teleparallel gravity and its effects
on the cosmic microwave background (CMB) anisotropy. The f (T) gravity generalizes the …
on the cosmic microwave background (CMB) anisotropy. The f (T) gravity generalizes the …