activity
20152026
most citedCMB-S4 Science Case, Reference Design, and Project Plan

443 citations · 1.4k across the 25 of their papers we have counts for

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Showing 2025Show all

6 papers · 1 filter

astro-ph.CO2025

A Multi-Probe ISW Study of Dark Energy Models with Negative Energy Density: Galaxy Correlations, Lensing Bispectrum, and Planck ISW-Lensing Likelihood

Payam Ghafari, Mahdi Najafi, Mina Ghodsi Yengejeh +3

We investigate the late-time imprints of three dark energy (DE) models, namely, the Chevallier-Polarski-Linder (CPL) parametrization, CDM, and an Omnipotent DE model, on…

astro-ph.CO2025

Nonlinear Matter Power Spectrum from relativistic -body Simulations: CDM versus CDM

Özgür Akarsu, Eleonora Di Valentino, Jiří Vyskočil +3

We present relativistic -body simulations of a CDM - sign-switching cosmological constant (CC) - scenario under general relativity and compare its nonlinear matter po…

astro-ph.CO2025

Constraining exotic high- reionization histories with Gaussian processes and the Cosmic Microwave Background

Hanyu Cheng, Ziwen Yin, Eleonora Di Valentino +2

The large-angle polarization anisotropies in the Cosmic Microwave Background (CMB) arise from Thomson scattering of CMB photons off free electrons in the post-recombination Univers…

astro-ph.CO2025

Cosmic Strings as Dynamical Dark Energy: Novel Constraints

Hanyu Cheng, Eleonora Di Valentino, Luca Visinelli

Cosmic strings, topological defects predicted by high-energy theories, may contribute to the late-time expansion of the Universe, effectively mimicking dynamical dark energy. We in…

astro-ph.CO2025

The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Eleonora Di Valentino, Jackson Levi Said, Adam Riess +533

The standard model of cosmology has provided a good phenomenological description of a wide range of observations both at astrophysical and cosmological scales for several decades.…

astro-ph.CO2025

Exploring the Growth-Index () Tension with CDM

Luis A. Escamilla, Özgür Akarsu, Eleonora Di Valentino +2

Recent observational analyses have revealed a significant tension in the growth index , which characterizes the growth rate of cosmic structures. Specifically, when treating