activity
20112023
most citedThe CLASSgal code for Relativistic Cosmological Large Scale Structure

150 citations · 826 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.CO2023★ 10 cited

The skewness of the distance-redshift relation in CDM

Tiziano Schiavone, Enea Di Dio, Giuseppe Fanizza

Starting from a recently proposed framework for the evaluation of the cosmological averages, we evaluate the higher-order moments for the distribution of a given observable. Then,…

gr-qc2023★ 1 cited

The Hawking Energy in a Perturbed Friedmann-Lemaître Universe

Dennis Stock, Enea Di Dio, Ruth Durrer

Hawking's quasi-local energy definition quantifies the energy enclosed by a spacelike 2-sphere in terms of the amount of lightbending on the sphere caused by the energy distributio…

astro-ph.CO2023★ 23 cited

Large Scale Limit of the Observed Galaxy Power Spectrum

Matteo Foglieni, Mattia Pantiri, Enea Di Dio +1

The large scale limit of the galaxy power spectrum provides a unique window into the early Universe through a possible detection of scale dependent bias produced by primordial non…

astro-ph.CO2023★ 12 cited

Wide-angle effects in the galaxy bispectrum

Kevin Pardede, Enea Di Dio, Emanuele Castorina

Primordial non-Gaussianities (PNG) leave unique signatures in the bispectrum of the large-scale structure. With upcoming galaxy surveys set to improve PNG constraints by at least o…

astro-ph.CO2022★ 1 cited

A smoking gun from the power spectrum dipole for elastic interactions in the dark sector

Jose Beltrán Jiménez, Enea Di Dio, David Figueruelo

Models with pure momentum exchange in the dark sector have been shown to provide a promising scenario to tackle the tension in the clustering inferred from high- and low-redshift p…

astro-ph.CO2022

The gauge invariant cosmological Jacobi map from weak lensing at leading order

Giuseppe Fanizza, Enea Di Dio, Ruth Durrer +1

We compute the weak lensing Jacobi map at first order in perturbation theory and show that it is both, gauge invariant and symmetric. Linear perturbations therefore do not induce a…

astro-ph.CO2021★ 69 cited

The observed galaxy power spectrum in General Relativity

Emanuele Castorina, Enea di Dio

Measurements of the clustering of galaxies in Fourier space, and at low wavenumbers, offer a window into the early Universe via the possible presence of scale dependent bias genera…

astro-ph.CO2019★ 14 cited

Rotation of the CMB polarisation by foreground lensing

Enea Di Dio, Ruth Durrer, Giuseppe Fanizza +1

We investigate the weak lensing corrections to the CMB polarization anisotropies. We concentrate on the effect of rotation and show that the rotation of polarisation is a true phys…

astro-ph.CO2016★ 32 cited

Impact of next-to-leading order contributions to CMB lensing

Giovanni Marozzi, Giuseppe Fanizza, Enea Di Dio +1

In this Letter we study the impact on cosmological parameter estimation, from present and future surveys, due to lensing corrections on CMB temperature and polarization anisotropie…

astro-ph.CO2016★ 40 cited

CMB-lensing beyond the leading order: temperature and polarization anisotropies

Giovanni Marozzi, Giuseppe Fanizza, Enea Di Dio +1

We investigate the weak lensing corrections to the CMB temperature and polarization anisotropies. We consider all the effects beyond the leading order: post-Born corrections, LSS c…

astro-ph.CO2016★ 45 cited

Non-Gaussianities due to Relativistic Corrections to the Observed Galaxy Bispectrum

E. Di Dio, H. Perrier, R. Durrer +4

High-precision constraints on primordial non-Gaussianity (PNG) will significantly improve our understanding of the physics of the early universe. Among all the subtleties in using…

astro-ph.CO2016★ 12 cited

Lensing smoothing of BAO wiggles

Enea Di Dio

We study non-perturbatively the effect of the deflection angle on the BAO wiggles of the matter power spectrum in real space. We show that from redshift z~2 this introduces a dispe…

astro-ph.CO2016★ 10 cited

The Alcock Paczynski test with Baryon Acoustic Oscillations: systematic effects for future surveys

Francesca Lepori, Enea Di Dio, Matteo Viel +2

We investigate the Alcock Paczynski (AP) test applied to the Baryon Acoustic Oscillation (BAO) feature in the galaxy correlation function. By using a general formalism that include…

astro-ph.CO2016★ 51 cited

CMB-lensing beyond the Born approximation

Giovanni Marozzi, Giuseppe Fanizza, Enea Di Dio +1

We investigate the weak lensing corrections to the cosmic microwave background temperature anisotropies considering effects beyond the Born approximation. To this aim, we use the s…

astro-ph.CO2015★ 69 cited

The bispectrum of relativistic galaxy number counts

Enea Di Dio, Ruth Durrer, Giovanni Marozzi +1

We discuss the dominant terms of the relativistic galaxy number counts to second order in cosmological perturbation theory on sub-Hubble scales and on intermediate to large redshif…

astro-ph.CO2015★ 28 cited

Relativistic effects in Lyman-alpha forest

Vid Iršič, Enea Di Dio, Matteo Viel

We present the calculation of the Lyman-alpha (Lyman-) transmitted flux fluctuations with full relativistic corrections to the first order. Even though several studies exist on…

astro-ph.CO2014★ 107 cited

Galaxy number counts to second order and their bispectrum

Enea Di Dio, Ruth Durrer, Giovanni Marozzi +1

We determine the number counts to second order in cosmological perturbation theory in the Poisson gauge and allowing for anisotropic stress. The calculation is performed using an i…

astro-ph.CO2014★ 20 cited

Distance-redshift relation in plane symmetric universes

Julian Adamek, Enea Di Dio, Ruth Durrer +1

Distance measurements are usually thought to probe the background metric of the universe, but in reality the presence of perturbations will lead to deviations from the result expec…

astro-ph.CO2013★ 72 cited

Cosmological Parameter Estimation with Large Scale Structure Observations

Enea Di Dio, Francesco Montanari, Ruth Durrer +1

We estimate the sensitivity of future galaxy surveys to cosmological parameters, using the redshift dependent angular power spectra of galaxy number counts, , calc…

astro-ph.CO2013★ 150 cited

The CLASSgal code for Relativistic Cosmological Large Scale Structure

Enea Di Dio, Francesco Montanari, Julien Lesgourgues +1

We present some accurate and efficient computations of large scale structure observables, obtained with a modified version of the CLASS code which is made publicly available. This…

hep-th2012★ 20 cited

A longitudinal gauge degree of freedom and the Pais Uhlenbeck field

Jose Beltrán Jiménez, Enea Di Dio, Ruth Durrer

We show that a longitudinal gauge degree of freedom for a vector field is equivalent to a Pais-Uhlenbeck scalar field. With the help of this equivalence, we can determine natural i…

astro-ph.CO2012★ 27 cited

Vector and Tensor Contributions to the Luminosity Distance

Enea Di Dio, Ruth Durrer

We compute the vector and tensor contributions to the luminosity distance fluctuations in first order perturbation theory and we expand them in spherical harmonics. This work prese…

astro-ph.CO2011★ 13 cited

Back Reaction from Walls

Enea Di Dio, Marc Vonlanthen, Ruth Durrer

We study the distance-redshift relation in a universe filled with 'walls' of pressure-less dust separated by under dense regions. We show that as long as the density contrast of th…