Shell-crossing in a ΛCDM Universe

Cornelius Rampf (Corresponding author), Oliver Hahn

Publications: Contribution to journalArticlePeer Reviewed

Abstract

Perturbation theory is an indispensable tool for studying the cosmic large-scale structure, and establishing its limits is therefore of utmost importance. One crucial limitation of perturbation theory is shell-crossing, which is the instance when cold-dark-matter trajectories intersect for the first time. We investigate Lagrangian perturbation theory (LPT) at very high orders in the vicinity of the first shell-crossing for random initial data in a realistic three-dimensional Universe. For this, we have numerically implemented the all-order recursion relations for the matter trajectories, from which the convergence of the LPT series at shell-crossing is established. Convergence studies performed at large orders reveal the nature of the convergence-limiting singularities. These singularities are not the well-known density singularities at shell-crossing but occur at later times when LPT already ceased to provide physically meaningful results.
Original languageEnglish
Pages (from-to)L71-L75
Number of pages5
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume501
Issue number1
DOIs
Publication statusPublished - Feb 2021

Austrian Fields of Science 2012

  • 103004 Astrophysics
  • 103044 Cosmology
  • 101028 Mathematical modelling

Keywords

  • cosmology
  • large-scale structure of universe
  • dark matter
  • MATTER
  • COLLAPSE
  • GRAVITATIONAL-INSTABILITY
  • large-scale structure of Universe
  • IMPROVED MODEL
  • NEWTONIAN COSMOLOGY
  • dark energy
  • PARTICLE TRAJECTORIES
  • cosmology: theory
  • Cosmology: theory
  • Dark matter
  • Dark energy
  • Large-scale structure of Universe

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