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20112026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 19.8k across the 136 of their papers we have counts for

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19 papers · 1 filter

astro-ph.CO2023★ 59 cited

A double take on early and interacting dark energy from JWST

Matteo Forconi, William Giarè, Olga Mena +4

The very first light captured by the James Webb Space Telescope (JWST) revealed a population of galaxies at very high redshifts more massive than expected in the canonical CDM m…

astro-ph.CO2023★ 33 cited

Measuring the reionization optical depth without large-scale CMB polarization

William Giarè, Eleonora Di Valentino, Alessandro Melchiorri

We study the possibility of measuring the optical depth at reionization, , without relying on large-scale Cosmic Microwave Background (CMB) polarization. Our analysis is driven…

astro-ph.CO2023★ 15 cited

Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions

William Giarè, Adrià Gómez-Valent, Eleonora Di Valentino +1

We study scatter-like interactions between neutrinos and dark matter in light of different combinations of temperature, polarization and lensing data released by three independent…

astro-ph.CO2023★ 6 cited

Possible Impact of non-Gaussianities on cosmological constraints in neutrino physics

Matteo Forconi, Eleonora Di Valentino, Alessandro Melchiorri +1

The search for non-Gaussian signatures in the Cosmic Microwave Background (CMB) is crucial for understanding the physics of the early Universe. Given the possibility of non-Gaussia…

astro-ph.CO2023★ 8 cited

Exploring Modified Gravity: Constraints on the and Parametrization with WMAP, ACT, and SPT

Uendert Andrade, Abraão J. S. Capistrano, Eleonora Di Valentino +1

The cosmic acceleration problem remains one of the most significant challenges in cosmology. One of the proposed solutions to this problem is the modification of gravity on large s…

astro-ph.CO2023★ 15 cited

CDM model: A promising scenario for alleviation of cosmological tensions

Ozgur Akarsu, Eleonora Di Valentino, Suresh Kumar +3

We present a comprehensive analysis of the CDM model, which explores the recent conjecture suggesting a rapid transition of the Universe from anti-de Sitter vacua to de…

astro-ph.CO2023★ 78 cited

The state of the dark energy equation of state circa 2023

Luis A. Escamilla, William Giarè, Eleonora Di Valentino +2

We critically examine the state of current constraints on the dark energy (DE) equation of state (EoS) . Our study is motivated by the observation that, while broadly consistent…

astro-ph.CO2023★ 13 cited

Lensing impact on cosmic relics and tensions

William Giarè, Olga Mena, Eleonora Di Valentino

Cosmological bounds on neutrinos and additional hypothetical light thermal relics, such as QCD axions, are currently among the most restrictive ones. These limits mainly rely on Co…

astro-ph.CO2023★ 18 cited

Tracking the Multifield Dynamics with Cosmological Data: A Monte Carlo approach

William Giarè, Mariaveronica De Angelis, Carsten van de Bruck +1

We introduce a numerical method specifically designed for investigating generic multifield models of inflation where a number of scalar fields are minimally coupled to gravit…

astro-ph.CO2023★ 75 cited

Omnipotent dark energy: A phenomenological answer to the Hubble tension

Shahnawaz A. Adil, Ozgur Akarsu, Eleonora Di Valentino +4

This paper introduces the class of omnipotent dark energy (DE) models characterized by nonmonotonic energy densities that are capable of attaining negative values with correspondin…

astro-ph.CO2023★ 16 cited

Exploring the Growth Index : Insights from Different CMB Dataset Combinations and Approaches

Enrico Specogna, Eleonora Di Valentino, Jackson Levi Said +1

In this study we investigate the growth index , which characterizes the growth of linear matter perturbations, while analysing different cosmological datasets. We compare the…

astro-ph.CO2023★ 76 cited

Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Luis A. Escamilla, Ozgur Akarsu, Eleonora Di Valentino +1

The cosmological dark sector remains an enigma, offering numerous possibilities for exploration. One particularly intriguing option is the (non-minimal) interaction scenario betwee…

astro-ph.CO2023★ 15 cited

Impact of the damping tail on neutrino mass constraints

Eleonora Di Valentino, Stefano Gariazzo, William Giarè +1

Model-independent mass limits assess the robustness of current cosmological measurements of the neutrino mass scale. Consistency between high-multipole and low-multiple Cosmic Micr…

astro-ph.CO2023★ 17 cited

Extended Analysis of Neutrino-Dark Matter Interactions with Small-Scale CMB Experiments

Philippe Brax, Carsten van de Bruck, Eleonora Di Valentino +2

We explore an extension of the standard CDM model by including an interaction between neutrinos and dark matter, and making use of the ground based telescope data of the Cosmic…

astro-ph.CO2023★ 11 cited

New insights on -DM Interactions

Philippe Brax, Carsten van de Bruck, Eleonora Di Valentino +2

We revisit the possibility of using cosmological observations to constrain models that involve interactions between neutrinos and dark matter. We show that small-scale measurements…

astro-ph.CO2023★ 76 cited

A Consistent View of Interacting Dark Energy from Multiple CMB Probes

Yuejia Zhai, William Giarè, Carsten van de Bruck +3

We analyze a cosmological model featuring an interaction between dark energy and dark matter in light of the measurements of the Cosmic Microwave Background released by three indep…

astro-ph.CO2023★ 12 cited

Exploring bulk viscous unified scenarios with Gravitational Waves Standard Sirens

Weiqiang Yang, Supriya Pan, Eleonora Di Valentino +2

We consider the unified bulk viscous scenarios and constrain them using the Cosmic Microwave Background observations from Planck 2018 and the Pantheon sample from Type Ia Supernova…

astro-ph.CO2023★ 19 cited

A New Test of Dynamical Dark Energy Models and Cosmic Tensions in Hořava Gravity

Eleonora Di Valentino, Nils A. Nilsson, Mu-In Park

Horava gravity has been proposed as a renormalizable, higher-derivative, Lorentz-violating quantum gravity model without ghost problems. A Horava gravity based dark energy (HDE) mo…

astro-ph.CO2023★ 97 cited

Exploring the tension and the evidence of dark sector interaction from 2D BAO measurements

Armando Bernui, Eleonora Di Valentino, William Giarè +2

We explore observational constraints on a cosmological model with an interaction between dark energy (DE) and dark matter (DM), using a compilation of 15 measurements of the 2D BAO…