The Atacama Cosmology Telescope: a measurement of the DR6 CMB lensing power spectrum and its implications for structure growth

FJ Qu, BD Sherwin, MS Madhavacheril… - The Astrophysical …, 2024 - iopscience.iop.org
We present new measurements of cosmic microwave background (CMB) lensing over 9400
deg 2 of the sky. These lensing measurements are derived from the Atacama Cosmology …

Quintessential interpretation of the evolving dark energy in light of DESI observations

Y Tada, T Terada - Physical Review D, 2024 - APS
The recent result of the Dark Energy Spectroscopic Instrument (DESI) in combination with
other cosmological data shows evidence of the evolving dark energy parametrized by the w …

Measurement of gravitational lensing of the cosmic microwave background using SPT-3G 2018 data

Z Pan, F Bianchini, WLK Wu, PAR Ade, Z Ahmed… - Physical Review D, 2023 - APS
We present a measurement of gravitational lensing over 1500 deg 2 of the Southern sky
using SPT-3G temperature data at 95 GHz and 150 GHz taken in 2018. The lensing …

Desi 2024 vi: Cosmological constraints from the measurements of baryon acoustic oscillations

AG Adame, J Aguilar, S Ahlen, S Alam… - arXiv preprint arXiv …, 2024 - arxiv.org
We present cosmological results from the measurement of baryon acoustic oscillations
(BAO) in galaxy, quasar and Lyman-$\alpha $ forest tracers from the first year of …

A non-linear solution to the S8 tension – II. Analysis of DES Year 3 cosmic shear

C Preston, A Amon, G Efstathiou - Monthly Notices of the Royal …, 2023 - academic.oup.com
Weak galaxy lensing surveys have consistently reported low values of the S 8 parameter
compared to the Planck lambda cold dark matter (ΛCDM) cosmology. Amon & Efstathiou …

Constraining cosmology with the Gaia-unWISE Quasar Catalog and CMB lensing: structure growth

D Alonso, G Fabbian, K Storey-Fisher… - … of Cosmology and …, 2023 - iopscience.iop.org
We study the angular clustering of Quaia, a Gaia-and unWISE-based catalog of over a
million quasars with an exceptionally well-defined selection function. With it, we derive …

Omnipotent dark energy: A phenomenological answer to the Hubble tension

SA Adil, Ö Akarsu, E Di Valentino, RC Nunes… - Physical Review D, 2024 - APS
This paper introduces the class of omnipotent dark energy (DE) models characterized by
nonmonotonic energy densities that are capable of attaining negative values with …

Observational constraints on dynamical dark energy models

O Avsajanishvili, GY Chitov, T Kahniashvili, S Mandal… - Universe, 2024 - mdpi.com
Scalar field ϕ CDM models provide an alternative to the standard Λ CDM paradigm, while
being physically better motivated. Dynamical scalar field ϕ CDM models are divided into two …

[HTML][HTML] PRyMordial: the first three minutes, within and beyond the standard model

AK Burns, TMP Tait, M Valli - The European Physical Journal C, 2024 - Springer
In this work we present PRyMordial: A package dedicated to efficient computations of
observables in the Early Universe with the focus on the cosmological era of Big Bang …

Inflationary potential as seen from different angles: model compatibility from multiple CMB missions

W Giarè, S Pan, E Di Valentino, W Yang… - … of Cosmology and …, 2023 - iopscience.iop.org
The cosmic microwave background (CMB) temperature and polarization anisotropies, as
observed by independent astronomical missions such as WMAP, Planck, and most recently …