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arxiv 1206.1225 v2 pith:IEPRE2LE submitted 2012-06-06 astro-ph.CO gr-qchep-ph

Cosmology and fundamental physics with the Euclid satellite

Luca Amendola , Stephen Appleby , David Bacon , Tessa Baker , Marco Baldi , Nicola Bartolo , Alain Blanchard , Camille Bonvin
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Stefano Borgani Enzo Branchini Clare Burrage Stefano Camera Carmelita Carbone Luciano Casarini Mark Cropper Claudia deRham Cinzia di Porto Anne Ealet Pedro G. Ferreira Fabio Finelli Juan Garcia-Bellido Tommaso Giannantonio Luigi Guzzo Alan Heavens Lavinia Heisenberg Catherine Heymans Henk Hoekstra Lukas Hollenstein Rory Holmes Ole Horst Knud Jahnke Thomas D. Kitching Tomi Koivisto Martin Kunz Giuseppe La Vacca Marisa March Elisabetta Majerotto Katarina Markovic David Marsh Federico Marulli Richard Massey Yannick Mellier David F. Mota Nelson Nunes Will Percival Valeria Pettorino Cristiano Porciani Claudia Quercellini Justin Read Massimiliano Rinaldi Domenico Sapone Roberto Scaramella Constantinos Skordis Fergus Simpson Andy Taylor Shaun Thomas Roberto Trotta Licia Verde Filippo Vernizzi Adrian Vollmer Yun Wang Jochen Weller Tom Zlosnik
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classification astro-ph.CO gr-qchep-ph
keywords euclidcosmologydarkcosmicenergyevolutionexpansionfundamental
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Euclid is a European Space Agency medium class mission selected for launch in 2019 within the Cosmic Vision 2015-2025 programme. 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 redshifts 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.

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Cited by 6 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

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    Joint kSZ-clustering analysis of ACT DR6 and CMASS yields a halo optical depth profile more extended than Websky simulations, suggesting stronger baryonic feedback.

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    Improved end-of-inflation dynamics shift the Starobinsky model's predicted spectral index n_s by up to 1.2×10^{-3} within the allowed reheating range.

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    Simulations in f(R) gravity show that environment density in the HOD model reduces assembly bias effects to 2-3% at z≲0.5 in both ΛCDM and modified gravity.

  6. Einstein or Jordan: seeking answers from the reheating constraints

    gr-qc 2019-07 unverdicted novelty 4.0

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