TY - UNPB
T1 - Euclid
T2 - Forecast constraints on consistency tests of the ΛCDM model
AU - Euclid Collaboration
AU - Nesseris, S.
AU - Sapone, D.
AU - Martinelli, M.
AU - Camarena, D.
AU - Marra, V.
AU - Sakr, Z.
AU - Garcia-Bellido, J.
AU - Valentijn, E. A.
PY - 2021/10/21
Y1 - 2021/10/21
N2 - The standard cosmological model is based on the simplifying assumptions
of a spatially homogeneous and isotropic universe on large scales. An
observational detection of their violation, at any redshift, would
immediately indicate the breakdown of the aforementioned assumptions or
presence of new physics. We quantify the ability of the Euclid mission,
together with contemporary surveys, to improve the current sensitivity
of null tests of the canonical cosmological constant and cold dark
matter (LCDM) model, in the redshift range $0
AB - The standard cosmological model is based on the simplifying assumptions
of a spatially homogeneous and isotropic universe on large scales. An
observational detection of their violation, at any redshift, would
immediately indicate the breakdown of the aforementioned assumptions or
presence of new physics. We quantify the ability of the Euclid mission,
together with contemporary surveys, to improve the current sensitivity
of null tests of the canonical cosmological constant and cold dark
matter (LCDM) model, in the redshift range $0
KW - Astrophysics - Cosmology and Nongalactic Astrophysics
KW - General Relativity and Quantum Cosmology
KW - High Energy Physics - Phenomenology
UR - http://adsabs.harvard.edu/abs/2021arXiv211011421N
U2 - 10.48550/arXiv.2110.11421
DO - 10.48550/arXiv.2110.11421
M3 - Preprint
BT - Euclid
PB - arXiv
ER -