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 …

Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

S Vagnozzi - Universe, 2023 - mdpi.com
The Hubble tension has now grown to a level of significance which can no longer be
ignored and calls for a solution which, despite a huge number of attempts, has so far eluded …

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 …

Hubble tension: The evidence of new physics

JP Hu, FY Wang - Universe, 2023 - mdpi.com
The Λ CDM model provides a good fit to most astronomical observations but harbors large
areas of phenomenology and ignorance. With the improvements in the precision and …

Consistency tests of from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension

S Vagnozzi - Physical Review D, 2021 - APS
New physics increasing the expansion rate just prior to recombination is among the least
unlikely solutions to the Hubble tension and would be expected to leave an important …

DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data

K Lodha, A Shafieloo, R Calderon, E Linder, W Sohn… - Physical Review D, 2025 - APS
Baryon acoustic oscillation data from the first year of the Dark Energy Spectroscopic
Instrument (DESI) provide near percent-level precision of cosmic distances in seven bins …

Relaxing cosmological tensions with a sign switching cosmological constant: Improved results with Planck, BAO, and Pantheon data

Ö Akarsu, S Kumar, E Özülker, JA Vazquez, A Yadav - Physical Review D, 2023 - APS
We present a further observational analysis of the Λ s CDM model proposed in Akarsu et
al.[Phys. Rev. D 104, 123512 (2021) PRVDAQ 2470-0010 10.1103/PhysRevD …

Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data

JQ Jiang, D Pedrotti, SS da Costa, S Vagnozzi - Physical Review D, 2024 - APS
We nonparametrically reconstruct the late-time expansion history in light of the latest baryon
acoustic oscillation (BAO) measurements from DESI combined with various type Ia …

Relaxing cosmological tensions with a sign switching cosmological constant

Ö Akarsu, S Kumar, E Özülker, JA Vazquez - Physical Review D, 2021 - APS
Inspired by the recent conjecture originated from graduated dark energy that the Universe
has recently transitioned from anti–de Sitter vacua to de Sitter vacua, we extend the …