Newtonian versus relativistic cosmology
arXiv:1207.2035 · doi:10.1103/PhysRevD.86.063527
Abstract
We show how the relativistic matter and velocity power spectra behave in different gauges. We construct a new gauge where both spectra coincide with Newtonian theory on all scales. However, in this gauge there are geometric quantities present which do not exist in Newtonian theory, for example the local variation of the Hubble parameter. Comparing this quantity to second order Newtonian quantities, we find that Newtonian theory is inaccurate on scales larger than 10 Mpc. This stresses the importance of relativistic corrections to Newtonian cosmological N-body simulations on these scales.
10 pages, 3 figures, accepted for publication in Physical Review D (Sept. 2012)
References in corpus (4)
- New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects
- A new framework for analyzing the effects of small scale inhomogeneities in cosmology
- On the dangers of using the growth equation on large scales in the Newtonian gauge
- The exact analytical solution of the linear structure growth rate in LCDM cosmology and its cosmological applications
Cited by in corpus (29)
- gevolution: a cosmological N-body code based on General Relativity
- Relativistic N-body simulations with massive neutrinos
- Fully relativistic treatment of light neutrinos in -body simulations
- Viscous dark matter growth in (neo-)Newtonian cosmology
- Relativistic Interpretation of Newtonian Simulations for Cosmic Structure Formation
- GRAMSES: a new route to general relativistic -body simulations in cosmology. Part I. Methodology and code description
- Relativistic numerical cosmology with Silent Universes
- The fully non-linear post-Friedmann frame-dragging vector potential: Magnitude and time evolution from N-body simulations
- Cosmology on all scales: a two-parameter perturbation expansion
- General relativistic 'screening' in cosmological simulations
- Accurate initial conditions in mixed Dark Matter--Baryon simulations
- Relativistic Lagrangian displacement field and tensor perturbations
- Dark energy perturbations in -body simulations
- Frame dragging and Eulerian frames in General Relativity
- Newton to Einstein - dust to dust
- The large-scale general-relativistic correction for Newtonian mocks
- Initial conditions for cosmological N-body simulations of the scalar sector of theories of Newtonian, Relativistic and Modified Gravity
- Simple expressions for second order density perturbations in standard cosmology
- GRAMSES: a new route to general relativistic -body simulations in cosmology. Part II. Initial conditions
- On the accuracy of N-body simulations at very large scales
- Dark energy homogeneity in general relativity: Are we applying it correctly?
- A Relativistic view on large scale N-body simulations
- Understanding the Dyer-Roeder approximation as a consequence of local cancellations of projected shear and expansion rate fluctuations
- Fully relativistic predictions in Horndeski gravity from standard Newtonian N-body simulations
- Large-scale imprint of relativistic effects in the cosmic magnification
- Perturbed redshifts from N-body simulations
- Relativistic rotation curve for cosmological structures
- Electrodynamics on Cosmological Scales
- Understanding the relativistic overdensity of galaxy surveys