Unveiling the singular dynamics in the cosmic large-scale structure

Author(s)
Cornelius Rampf, Uriel Frisch, Oliver Hahn
Abstract

It is known that the gravitational collapse of cold dark matter leads to infinite-density caustics that seed the primordial dark-matter haloes in the large-scale structure. The development of these caustics begins, generically, as an almost one-dimensional phenomenon with the formation of pancakes. Focusing on the one-dimensional case, we identify a landscape of non-differentiable, and thus, singular features in the particle acceleration that emerge after the first crossing of particle trajectories. We complement our fully analytical studies by high-resolution simulations and find outstanding agreement, particularly shortly after the first crossing. We develop the methods in one space dimension but outline briefly the necessary steps for the 3D case.

Organisation(s)
Department of Mathematics, Department of Astrophysics
External organisation(s)
Université Côte d'Azur
Journal
Monthly Notices of the Royal Astronomical Society: Letters
Volume
505
Pages
L90-L94
No. of pages
5
ISSN
1745-3925
DOI
https://doi.org/10.1093/mnrasl/slab053
Publication date
07-2021
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics, 103038 Space exploration, 103044 Cosmology
Keywords
Portal url
https://ucrisportal.univie.ac.at/en/publications/b5da70fd-40de-4403-85d5-c525c6df905f