Non-linear vorticity-density coupling in Lagrangian dynamics
arXiv:astro-ph/9711252 · doi:10.1143/PTP.99.585
Abstract
We present a general Lagrangian formalism that allows the treatment of vorticity. We give solutions for the rotational perturbations up to the third-order in a flat background universe. We show how the primordial vorticity affects the evolution of the density fluctuation in high-density regions.
15 pages; submitted to Progress of Theoretical Physics
Cited by in corpus (14)
- Ellipsoidal collapse and previrialization
- On the evolution of aspherical perturbations in the universe: an analytical model
- Extending Lagrangian perturbation theory to a fluid with velocity dispersion
- Transients from initial conditions based on Lagrangian perturbation theory in N-body simulations
- Third-order perturbative solutions in the Lagrangian perturbation theory with pressure
- Lagrangian description of the fluid flow with vorticity in the relativistic cosmology
- Improving the Lagrangian perturbative solution for cosmic fluid: Applying Shanks transformation
- Correspondence between the adhesion model and the velocity dispersion for the cosmological fluid
- Performance of the optimized Post-Zel'dovich approximation for CDM models in arbitrary FLRW cosmologies
- Third-order perturbative solutions in the Lagrangian perturbation theory with pressure II: Effect of the transverse modes
- Transients from initial conditions based on Lagrangian perturbation theory in -body simulations II: the effect of the transverse mode
- Fourth-order perturbative equations in Lagrangian perturbation theory for a cosmological dust fluid
- Scaling Relations for Collision-less Dark Matter Turbulence
- Transients from Initial Conditions Based on Lagrangian Perturbation Theory in -body Simulations III: The Case of GADGET-2 Code