A few numbers from the turnaround epoch of collapse
Abstract
The turnaround epoch of gravitational collapse is examined by means of relativistic Lagrangian perturbation theory. Averaged, scalar equations applied to the fluid's evolution reveal some scaleindependent universality of parameters for a wide variety of initial conditions. In particular, the density contrast of the collapsing domain at the turnaround is shown to be significantly smaller than the value provided by Eulerian perturbative (homogeneous and spherical) model. Combined curvature and kinematical backreaction are shown to be of the order of the energy density. Possible improvements of our treatment are put into perspective.
 Publication:

arXiv eprints
 Pub Date:
 December 2019
 arXiv:
 arXiv:1912.12683
 Bibcode:
 2019arXiv191212683O
 Keywords:

 General Relativity and Quantum Cosmology
 EPrint:
 4 pages,contribution to the proceedings of The 6th Conference of the Polish Society on Relativity