Is the observable Universe consistent with the cosmological principle?

PK Aluri, P Cea, P Chingangbam… - … and Quantum Gravity, 2023 - iopscience.iop.org
The cosmological principle (CP)—the notion that the Universe is spatially isotropic and
homogeneous on large scales—underlies a century of progress in cosmology. It is …

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) …

Hubble parameter measurement constraints on the redshift of the deceleration–acceleration transition, dynamical dark energy, and space curvature

O Farooq, FR Madiyar, S Crandall… - The Astrophysical …, 2017 - iopscience.iop.org
We compile an updated list of 38 measurements of the Hubble parameter H (z) between
redshifts 0.07≤ z≤ 2.36 and use them to place constraints on model parameters of constant …

Non-parametric spatial curvature inference using late-Universe cosmological probes

S Dhawan, J Alsing, S Vagnozzi - Monthly Notices of the Royal …, 2021 - academic.oup.com
Inferring high-fidelity constraints on the spatial curvature parameter, ΩK, under as few
assumptions as possible, is of fundamental importance in cosmology. We propose a method …

Cosmic chronometers to calibrate the ladders and measure the curvature of the Universe. A model-independent study

A Favale, A Gómez-Valent… - Monthly Notices of the …, 2023 - academic.oup.com
We use the state-of-the-art data on cosmic chronometers (CCH) and the Pantheon+
compilation of supernovae of Type Ia (SNIa) to test the constancy of the SNIa absolute …

The galaxy power spectrum take on spatial curvature and cosmic concordance

S Vagnozzi, E Di Valentino, S Gariazzo… - Physics of the Dark …, 2021 - Elsevier
The concordance of the Λ CDM cosmological model in light of current observations has
been the subject of an intense debate in recent months. The 2018 Planck Cosmic …

Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters

N Khadka, B Ratra - Monthly Notices of the Royal Astronomical …, 2021 - academic.oup.com
We use six different cosmological models to study the recently released compilation of X-ray
and UV flux measurements of 2038 quasars (QSOs) which span the redshift range 0.009≤ …

The Cardassian expansion revisited: constraints from updated Hubble parameter measurements and type Ia supernova data

J Magana, MH Amante… - Monthly Notices of the …, 2018 - academic.oup.com
Motivated by an updated compilation of observational Hubble data (OHD) that consist of 51
points in the redshift range of 0.07< z< 2.36, we study an interesting model known as …

Baryon acoustic oscillation, Hubble parameter, and angular size measurement constraints on the Hubble constant, dark energy dynamics, and spatial curvature

J Ryan, Y Chen, B Ratra - Monthly Notices of the Royal …, 2019 - academic.oup.com
In this paper, we use all available baryon acoustic oscillation, Hubble parameter, and
quasar angular size data to constrain six dark energy cosmological models, both spatially …

Using quasar X-ray and UV flux measurements to constrain cosmological model parameters

N Khadka, B Ratra - Monthly Notices of the Royal Astronomical …, 2020 - academic.oup.com
Risaliti and Lusso have compiled X-ray and UV flux measurements of 1598 quasars (QSOs)
in the redshift range 0.036≤ z≤ 5.1003, part of which, z∼ 2.4− 5.1, is largely …