Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies

E Abdalla, GF Abellán, A Aboubrahim, A Agnello… - Journal of High Energy …, 2022 - Elsevier
Abstract The standard Λ Cold Dark Matter (ΛCDM) cosmological model provides a good
description of a wide range of astrophysical and cosmological data. However, there are a …

In the realm of the Hubble tension—a review of solutions

E Di Valentino, O Mena, S Pan, L Visinelli… - … and Quantum Gravity, 2021 - iopscience.iop.org
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 …

Finite-time cosmological singularities and the possible fate of the Universe

J de Haro, S Nojiri, SD Odintsov, VK Oikonomou, S Pan - Physics Reports, 2023 - Elsevier
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 …

Nonminimal dark sector physics and cosmological tensions

E Di Valentino, A Melchiorri, O Mena, S Vagnozzi - Physical Review D, 2020 - APS
We explore whether nonstandard dark sector physics might be required to solve the existing
cosmological tensions. The properties we consider in combination are (a) an interaction …

Interacting dark energy in the early 2020s: A promising solution to the H0 and cosmic shear tensions

E Di Valentino, A Melchiorri, O Mena… - Physics of the Dark …, 2020 - Elsevier
We examine interactions between dark matter and dark energy in light of the latest
cosmological observations, focusing on a specific model with coupling proportional to the …

Eppur è piatto? The cosmic chronometers take on spatial curvature and cosmic concordance

S Vagnozzi, A Loeb, M Moresco - The Astrophysical Journal, 2021 - iopscience.iop.org
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 …

New tests of dark sector interactions from the full-shape galaxy power spectrum

RC Nunes, S Vagnozzi, S Kumar, E Di Valentino… - Physical Review D, 2022 - APS
We explore the role of redshift-space galaxy clustering data in constraining nongravitational
interactions between dark energy (DE) and dark matter (DM), for which state-of-the-art limits …

Tale of stable interacting dark energy, observational signatures, and the H0 tension

W Yang, S Pan, E Di Valentino… - … of Cosmology and …, 2018 - iopscience.iop.org
We investigate the observational consequences of a novel class of stable interacting dark
energy (IDE) models, featuring interactions between dark matter (DM) and dark energy (DE) …

Echo of interactions in the dark sector

S Kumar, RC Nunes - Physical Review D, 2017 - APS
We investigate the observational constraints on an interacting vacuum energy scenario with
two different neutrino schemes (with and without a sterile neutrino) using the most recent …

Interacting scenarios with dynamical dark energy: Observational constraints and alleviation of the tension

S Pan, W Yang, E Di Valentino, EN Saridakis… - Physical Review D, 2019 - APS
We investigate interacting scenarios that belong to a wider class, since they include a
dynamical dark energy component whose equation of state follows various one-parameter …