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 …
Nonminimal dark sector physics and cosmological tensions
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 …
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
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 …
cosmological observations, focusing on a specific model with coupling proportional to the …
Tale of stable interacting dark energy, observational signatures, and the H0 tension
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) …
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
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 …
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
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 …
corresponding to a well-known interacting dark energy model discussed in the literature …
Reconciling CMB and structure growth measurements with dark energy interactions
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 …
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
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 …
inferred from observations of the cosmic microwave background (CMB) assuming the …
Dark sectors with dynamical coupling
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 …
which controls the strength of their interaction. While this coupling is commonly assumed to …