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NLO-CO SIGNED

Large scale structure of the Universe and fundamental physics

Total Cost €

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EC-Contrib. €

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Partnership

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Project "NLO-CO" data sheet

The following table provides information about the project.

Coordinator
COMMISSARIAT A L ENERGIE ATOMIQUE ET AUX ENERGIES ALTERNATIVES 

Organization address
address: RUE LEBLANC 25
city: PARIS 15
postcode: 75015
website: www.cea.fr

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country France [FR]
 Project website http://miguelzuma.github.io/
 Total cost 264˙668 €
 EC max contribution 264˙668 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2015
 Funding Scheme MSCA-IF-GF
 Starting year 2017
 Duration (year-month-day) from 2017-11-01   to  2020-10-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    COMMISSARIAT A L ENERGIE ATOMIQUE ET AUX ENERGIES ALTERNATIVES FR (PARIS 15) coordinator 264˙668.00
2    THE REGENTS OF THE UNIVERSITY OF CALIFORNIA US (OAKLAND CA) partner 0.00

Map

 Project objective

The purpose of this cosmology project is to study the content and evolution of our Universe using the distribution of matter on large scales. A key goal of forthcoming galaxy surveys is probing fundamental physics, such as the mass of neutrinos and the nature of dark energy, the component sourcing cosmic acceleration. The analysis and interpretation of their data crucially relies on the development of perturbation theory methods and other theoretical tools to describe and predict the evolution of large scale structures in the universe, particularly in the non-linear regime. This project aims to establish the optimal approach to compute the growth of structures and to extract information about dark energy and neutrino masses from the data.

This action will address important questions in non-linear structure formation. More specifically, I will 1) devise efficient techniques to obtain information on non-linear clustering from data and apply it to bispectrum estimators and BAO reconstruction; 2) obtain the predictions for general massive neutrinos and dark energy models, beyond the power spectrum; and 3) improve the precision of semi-analytical methods to compute non-linear perturbations on small scales; A very concrete goal of the project is to produce a numerical code and make it public. This code will find direct application in the forecast and analysis of the data from the Euclid mission and other galaxy surveys, to probe the properties of neutrinos and the nature of gravity.

In the outgoing phase I will work at University of California, Berkeley (US) to benefit from its great involvement in galaxy surveys and expertise in studies of large scale structure in connection to observations. In the return phase I will work in the Institut de Physique Théorique Saclay (France) where many theoretical developments in perturbation theory and extensions to non-standard models have been developed.

 Publications

year authors and title journal last update
List of publications.
2018 E. Bellini, A. Barreira, N. Frusciante, B. Hu, S. Peirone, M. Raveri, M. Zumalacárregui, A. Avilez-Lopez, M. Ballardini, R. A. Battye, B. Bolliet, E. Calabrese, Y. Dirian, P. G. Ferreira, F. Finelli, Z. Huang, M. M. Ivanov, J. Lesgourgues, B. Li, N. A. Lima, F. Pace, D. Paoletti, I. Sawicki, A. Silvestri, C. Skordis, C. Umiltà, F. Vernizzi
Comparison of Einstein-Boltzmann solvers for testing general relativity
published pages: , ISSN: 2470-0010, DOI: 10.1103/physrevd.97.023520
Physical Review D 97/2 2020-04-24
2018 Carlos García-García, Eric V. Linder, Pilar Ruíz-Lapuente, Miguel Zumalacárregui
Dark energy from α-attractors: phenomenology and observational constraints
published pages: 022-022, ISSN: 1475-7516, DOI: 10.1088/1475-7516/2018/08/022
Journal of Cosmology and Astroparticle Physics 2018/08 2020-04-24
2018 A Spurio Mancini, R Reischke, V Pettorino, B M Schäfer, M Zumalacárregui
Testing (modified) gravity with 3D and tomographic cosmic shear
published pages: 3725-3738, ISSN: 0035-8711, DOI: 10.1093/mnras/sty2092
Monthly Notices of the Royal Astronomical Society 480/3 2020-04-24
2018 Miguel Zumalacárregui, Uroš Seljak
Limits on Stellar-Mass Compact Objects as Dark Matter from Gravitational Lensing of Type Ia Supernovae
published pages: , ISSN: 0031-9007, DOI: 10.1103/physrevlett.121.141101
Physical Review Letters 121/14 2020-04-24
2017 Miguel Zumalacárregui, Emilio Bellini, Ignacy Sawicki, Julien Lesgourgues, Pedro G. Ferreira
hi_class: Horndeski in the Cosmic Linear Anisotropy Solving System
published pages: 019-019, ISSN: 1475-7516, DOI: 10.1088/1475-7516/2017/08/019
Journal of Cosmology and Astroparticle Physics 2017/08 2020-04-24
2018 Jose María Ezquiaga, Miguel Zumalacárregui
Dark Energy in Light of Multi-Messenger Gravitational-Wave Astronomy
published pages: , ISSN: 2296-987X, DOI: 10.3389/fspas.2018.00044
Frontiers in Astronomy and Space Sciences 5 2020-04-24
2019 Micah Brush, Eric V. Linder, Miguel Zumalacárregui
No Slip CMB
published pages: 029-029, ISSN: 1475-7516, DOI: 10.1088/1475-7516/2019/01/029
Journal of Cosmology and Astroparticle Physics 2019/01 2020-04-24

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