The Cosmological Consistency Relation in a Universe with Structure
arXiv:1907.11101 · doi:10.1088/1475-7516/2019/12/034
Abstract
In this short paper we determine the effects of structure on the cosmological consistency relation which is valid in a perfect Friedmann Universe. We show that within CDM the consistency relation is violated by about 1.5% for redshifts and this violation raises up to 2% at and 3% at after which it settles at about 2.7% for . This effect of cosmic structure on the distance redshift relation is also very sensitive to the determination of the dark energy equation of state via cosmic distances. It actually leads to an apparent unphysical behavior of which even diverges at and which we also discuss here.
arXiv comment11 pages, 3 figures, version accepted for publication in JCAP
References in corpus (17)
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1
- The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview
- Extended Limber Approximation
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z=0.57 from anisotropic clustering
- A general test of the Copernican Principle
- Fluctuations of the luminosity distance
- Dynamical Dark Energy or Simply Cosmic Curvature?
- Average and dispersion of the luminosity-redshift relation in the concordance model
- An exact Jacobi map in the geodesic light-cone gauge
- The second-order luminosity-redshift relation in a generic inhomogeneous cosmology
- Nonlinear relativistic corrections to cosmological distances, redshift and gravitational lensing magnification. I - Key results
- Nonlinear relativistic corrections to cosmological distances, redshift and gravitational lensing magnification. II - Derivation
- The luminosity distance-redshift relation up to second order in the Poisson gauge with anisotropic stress
- A new method for the Alcock-Paczynski test
- What is the distance to the CMB?
- The Alcock Paczynski test with Baryon Acoustic Oscillations: systematic effects for future surveys