Cosmology and fundamental physics with the Euclid satellite
Author
dc.contributor.author
Amendola, Luca
Author
dc.contributor.author
Sapone, Domenico
Admission date
dc.date.accessioned
2018-08-16T14:06:02Z
Available date
dc.date.available
2018-08-16T14:06:02Z
Publication date
dc.date.issued
2018
Cita de ítem
dc.identifier.citation
Living Reviews in Relativity Volumen: 21 Páginas: 1-345 Número de artículo: 2
es_ES
Identifier
dc.identifier.other
10.1007/s41114-017-0010-3
Identifier
dc.identifier.uri
https://repositorio.uchile.cl/handle/2250/150985
Abstract
dc.description.abstract
Euclid is a European Space Agency medium-class mission selected for launch in 2020 within the cosmic vision 2015-2025 program. The main goal of Euclid is to understand the origin of the accelerated expansion of the universe. Euclid will explore the expansion history of the universe and the evolution of cosmic structures by measuring shapes and red-shifts of galaxies as well as the distribution of clusters of galaxies over a large fraction of the sky. Although the main driver for Euclid is the nature of dark energy, Euclid science covers a vast range of topics, from cosmology to galaxy evolution to planetary research. In this review we focus on cosmology and fundamental physics, with a strong emphasis on science beyond the current standard models. We discuss five broad topics: dark energy and modified gravity, dark matter, initial conditions, basic assumptions and questions of methodology in the data analysis. This review has been planned and carried out within Euclid's Theory Working Group and is meant to provide a guide to the scientific themes that will underlie the activity of the group during the preparation of the Euclid mission.
es_ES
Patrocinador
dc.description.sponsorship
MIUR
ERC
280127
693024
FCT - FCT/MCTES (Portugal)
IF/00064/2012
POPH/FSE (EC)
Transregio Grant on 'The Dark Universe'
TRR33
Department of Energy
DE-SC0009946
research agency CNPq
ESIF
MEYS
CoGraDS-CZ.02.1.01/0.0/0.0/15_003/0000437
Italian Ministry for Education, University and Research (MIUR) through the SIR individual grant SIMCODE
RBSI14P4IH
Fondecyt
11140496
Research Council of Norway
NASA ROSES
12-EUCLID12-0004