activity
20182026
most citedThe kinematic Sunyaev-Zel'dovich effect of the large-scale structure (II): the effect of modified gravity

11 citations · 21 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2026

MG-NECOLA: A Field-Level Emulator for Gravity and Massive Neutrino Cosmologies

J. Bayron Orjuela-Quintana, Mauricio Reyes, Elena Giusarma +3

Accurate modeling of non-linear gravitational dynamics is essential for constraining extensions to the standard cosmological model using large-scale structure observations. While h…

astro-ph.CO2026

Field-Level Inference of Primordial Non-Gaussianity with the Quijote Simulation Suite

Adam Andrews, Jens Jasche, Guilhem Lavaux +10

Local primordial non-Gaussianity, parameterised as , will be stringently constrained using state-of-the-art methods applied to next-generation galaxy redshi…

astro-ph.CO2025

: Accurate non-Gaussian initial conditions with arbitrary bispectrum for N-body simulations

Emanuele Fondi, Licia Verde, Marco Baldi +3

Primordial non-Gaussianity is predicted by various inflationary models, and N-body simulations are a crucial tool for studying its imprints on large-scale structure. In this work,…

astro-ph.CO2024

Probing massive neutrinos and modified gravity with redshift-space morphologies and anisotropies of large-scale structure

Wei Liu, Liang Wu, Francisco Villaescusa-Navarro +3

Strong degeneracy exists between some modified gravity (MG) models and massive neutrinos because the enhanced structure growth produced by modified gravity can be suppressed due to…

astro-ph.CO2024

The constraining power of the Marked Power Spectrum: an analytical study

Marco Marinucci, Gabriel Jung, Michele Liguori +8

The marked power spectrum - a two-point correlation function of a transformed density field - has emerged as a promising tool for extracting cosmological information from the large…

astro-ph.CO2024

A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity

Luca Fiorino, Sofia Contarini, Federico Marulli +4

We investigate the effect of primordial non-Gaussianities on halo number counts using N-body simulations with different values of . We show how current theore…

astro-ph.CO2024★ 10 cited

Towards unveiling the large-scale nature of gravity with the wavelet scattering transform

Georgios Valogiannis, Francisco Villaescusa-Navarro, Marco Baldi

We present the first application of the Wavelet Scattering Transform (WST) in order to constrain the nature of gravity using the three-dimensional (3D) large-scale structure of the…

astro-ph.CO2024

Cosmological simulations of scale-dependent primordial non-Gaussianity

Marco Baldi, Emanuele Fondi, Dionysios Karagiannis +9

We present the results of a set of cosmological N-body simulations with standard CDM cosmology but characterized by a scale-dependent primordial non-Gaussianity of the local typ…

astro-ph.CO2024

Quijote-PNG: Optimizing the summary statistics to measure Primordial non-Gaussianity

Gabriel Jung, Andrea Ravenni, Michele Liguori +4

We apply a suite of different estimators to the Quijote-PNG halo catalogues to find the best approach to constrain Primordial non-Gaussianity (PNG) at non-linear cosmological scale…

astro-ph.CO2018★ 11 cited

The kinematic Sunyaev-Zel'dovich effect of the large-scale structure (II): the effect of modified gravity

M. Roncarelli, M. Baldi, F. Villaescusa-Navarro

The key to understand the nature of dark energy relies in our ability to probe the distant Universe. In this framework, the recent detection of the kinematic Sunyaev-Zel'dovich (kS…