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 …

Challenges for ΛCDM: An update

L Perivolaropoulos, F Skara - New Astronomy Reviews, 2022 - Elsevier
A number of challenges to the standard Λ CDM model have been emerging during the past
few years as the accuracy of cosmological observations improves. In this review we discuss …

On the Hubble constant tension in the SNe Ia Pantheon sample

MG Dainotti, B De Simone, T Schiavone… - The Astrophysical …, 2021 - iopscience.iop.org
On the Hubble Constant Tension in the SNe Ia Pantheon Sample - IOPscience This site uses
cookies. By continuing to use this site you agree to our use of cookies. To find out more, see …

Cosmology intertwined III: fσ8 and S8

E Di Valentino, LA Anchordoqui, Ö Akarsu… - Astroparticle …, 2021 - Elsevier
Abstract The standard Λ Cold Dark Matter cosmological model provides a wonderful fit to
current cosmological data, but a few statistically significant tensions and anomalies were …

Arbitrating the S8 discrepancy with growth rate measurements from redshift-space distortions

RC Nunes, S Vagnozzi - Monthly Notices of the Royal …, 2021 - academic.oup.com
Within the Lambda cold dark matter (ΛCDM) model, measurements from recent cosmic
microwave background (CMB) and weak lensing (WL) surveys have uncovered a∼ 3σ …

Can late-time extensions solve the and tensions?

L Heisenberg, H Villarrubia-Rojo, J Zosso - Physical Review D, 2022 - APS
We analyze the properties that any late-time modification of the Λ CDM expansion history
must have in order to consistently solve both the H 0 and the σ 8 tensions. Taking a model …

tension, phantom dark energy, and cosmological parameter degeneracies

G Alestas, L Kazantzidis, L Perivolaropoulos - Physical Review D, 2020 - APS
Phantom dark energy (w<-1) can produce amplified cosmic acceleration at late times, thus
increasing the value of H 0 favored by CMB data and releasing the tension with local …

Testing F (Q) gravity with redshift space distortions

BJ Barros, T Barreiro, T Koivisto, NJ Nunes - Physics of the Dark Universe, 2020 - Elsevier
A Bayesian statistical analysis using redshift space distortions data is performed to test a
model of Symmetric Teleparallel Gravity where gravity is non-metrical. The cosmological …

Thermodynamic parametrization of dark energy

S Capozziello, R D'Agostino, O Luongo - Physics of the Dark Universe, 2022 - Elsevier
We propose a new parametrization of dark energy motivated by thermodynamics. To this
aim, we consider Padé polynomials to reconstruct the form of deceleration parameter …

Simultaneously solving the H0 and σ8 tensions with late dark energy

L Heisenberg, H Villarrubia-Rojo, J Zosso - Physics of the Dark Universe, 2023 - Elsevier
In a model independent approach, we derive generic conditions that any late time
modification of the Λ CDM expansion history must satisfy in order to consistently solve both …