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 …

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) …

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 …

Late-time constraints on interacting dark energy: Analysis independent of H0, rd, and MB

D Benisty, S Pan, D Staicova, E Di Valentino… - Astronomy & …, 2024 - aanda.org
We investigated a possible interaction between cold dark matter and dark energy,
corresponding to a well-known interacting dark energy model discussed in the literature …

Reconciling CMB and structure growth measurements with dark energy interactions

A Pourtsidou, T Tram - Physical Review D, 2016 - APS
We study a coupled quintessence model with pure momentum exchange and present the
effects of such an interaction on the cosmic microwave background (CMB) and matter power …

[HTML][HTML] Dissecting the H0 and S8 tensions with Planck+ BAO+ supernova type Ia in multi-parameter cosmologies

LA Anchordoqui, E Di Valentino, S Pan… - Journal of High Energy …, 2021 - Elsevier
The mismatch between the locally measured expansion rate of the universe and the one
inferred from observations of the cosmic microwave background (CMB) assuming the …

Dark sectors with dynamical coupling

W Yang, O Mena, S Pan, E Di Valentino - Physical Review D, 2019 - APS
Coupled dark matter–dark energy scenarios are modeled via a dimensionless parameter ξ,
which controls the strength of their interaction. While this coupling is commonly assumed to …