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 …

Observational probes of cosmic acceleration

DH Weinberg, MJ Mortonson, DJ Eisenstein, C Hirata… - Physics reports, 2013 - Elsevier
The accelerating expansion of the universe is the most surprising cosmological discovery in
many decades, implying that the universe is dominated by some form of “dark energy” with …

DESI 2024: reconstructing dark energy using crossing statistics with DESI DR1 BAO data

R Calderon, K Lodha, A Shafieloo… - … of Cosmology and …, 2024 - iopscience.iop.org
Abstract We implement Crossing Statistics to reconstruct in a model-agnostic manner the
expansion history of the universe and properties of dark energy, using DESI Data Release 1 …

Revealing intrinsic flat biases with standardizable candles

E Ó Colgáin, MM Sheikh-Jabbari, R Solomon… - Physical Review D, 2022 - APS
Emerging high-redshift cosmological probes, in particular quasars (QSOs), show a
preference for larger matter densities, Ω m≈ 1, within the flat Λ CDM framework. Here, using …

Hubble parameter and Baryon Acoustic Oscillation measurement constraints on the Hubble constant, the deviation from the spatially flat ΛCDM model, the …

H Yu, B Ratra, FY Wang - The Astrophysical Journal, 2018 - iopscience.iop.org
We compile a complete collection of reliable Hubble parameter H (z) data to redshift z≤
2.36 and use them with the Gaussian Process method to determine continuous H (z) …

On the impact of f(Q) gravity on the large scale structure

O Sokoliuk, S Arora, S Praharaj… - Monthly Notices of …, 2023 - academic.oup.com
We investigate the exponential f (Q) symmetric teleparallel gravitation, namely using ME-
GADGET code to probe the structure formation with box sizes L Box= 10/100 Mpc h–1 and …

[HTML][HTML] Cosmology in f (R, Lm) gravity

LV Jaybhaye, R Solanki, S Mandal, PK Sahoo - Physics Letters B, 2022 - Elsevier
In this letter, we investigate the cosmic expansion scenario of the universe in the framework
of f (R, L m) gravity theory. We consider a non-linear f (R, L m) model, specifically, f (R, L m) …

Model-independent cosmological inference post DESI DR1 BAO measurements

P Mukherjee, AA Sen - Physical Review D, 2024 - APS
In this work, we implement Gaussian process regression to reconstruct the expansion history
of the Universe in a model-agnostic manner, using the Pantheon-Plus SN-Ia compilation in …

Running Hubble tension and a H0 diagnostic

C Krishnan, E Ó Colgáin, MM Sheikh-Jabbari, T Yang - Physical Review D, 2021 - APS
Hubble tension is routinely presented as a mismatch between the Hubble constant H 0
determined locally and a value inferred from the flat Λ CDM cosmology. In essence, the …

Dark energy

M Li, XD Li, S Wang, Y Wang - Communications in theoretical …, 2011 - iopscience.iop.org
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