A relativistic approach to nonlinear peculiar velocities and the Zeldovich approximation
arXiv:astro-ph/0209143 · doi:10.1103/PhysRevD.66.124015
Abstract
We study the peculiar motion of non-relativistic matter in a fully covariant way. The exact nonlinear equations are derived and then applied to the case of pressure-free matter, moving relatively to a quasi-Newtonian Eulerian frame. Our two-frame formalism facilitates the study of the nonlinear kinematics of the matter, as the latter decouples from the background expansion and starts to ``turn around'' and collapse. Applied to second perturbative order, our equations provide a fully covariant formulation of the Zeldovich approximation, which by construction addresses the mildly nonlinear regime of structure formation. Employing a dynamical system approach, we show that, just like in the Newtonian case, the relativistic treatment also predicts that pancakes are the natural end-structures for any generic overdensity.
Minor changes, accepted by Phys. Rev. D
References in corpus (1)
Cited by in corpus (24)
- Relativistic cosmology and large-scale structure
- Cosmology with inhomogeneous magnetic fields
- Resembling dark energy and modified gravity with Finsler-Randers cosmology
- Applicability of the linearly perturbed FRW metric and Newtonian cosmology
- Lagrangian theory of structure formation in relativistic cosmology I: Lagrangian framework and definition of a nonperturbative approximation
- Peculiar motions, accelerated expansion and the cosmological axis
- Light propagation and the average expansion rate in near-FRW universes
- Relativistic numerical cosmology with Silent Universes
- The deceleration parameter in `tilted' Friedmann universes
- Multiple non-spherical structures from the extrema of Szekeres scalars
- Zel'dovich approximation and General Relativity
- Coarse-grained description of cosmic structure from Szekeres models
- The peculiar Raychaudhuri equation
- The deceleration parameter in `tilted' universes: generalising the Friedmann background
- Large-scale peculiar motions and cosmic acceleration
- Relativistic approach to the kinematics of large-scale peculiar motions
- Cosmic microwave background with Brans-Dicke Gravity: I. Covariant Formulation
- Replacing dark energy by silent virialisation
- Emergence of spatial curvature
- Large-scale peculiar velocity fields: Newtonian vs relativistic treatment
- Peculiar velocity measurement in a clumpy universe
- Lagrangian theory of structure formation in relativistic cosmology. V. Irrotational fluids
- Covariant Evolution of Gravitoelectromagnetism
- Modified first law of charged dilaton black hole