Relativistic initial conditions for N-body simulations
From MaRDI portal
Publication:5024214
DOI10.1088/1475-7516/2017/06/043OpenAlexW2590840589MaRDI QIDQ5024214
David Wands, Robert G. Crittenden, Christian Fidler, Thomas Tram, Kazuya Koyama, Cornelius Rampf
Publication date: 28 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1702.03221
Related Items (12)
A minimal model for massive neutrinos in Newtonian N-body simulations ⋮ Fully relativistic predictions in Horndeski gravity from standard Newtonian N-body simulations ⋮ Does spatial flatness forbid the turnaround epoch of collapsing structures? ⋮ General relativistic cosmological N-body simulations. Part I. Time integration ⋮ GRAMSES: a new route to general relativistic N-body simulations in cosmology. Part I. Methodology and code description ⋮ GRAMSES: a new route to general relativistic N-body simulations in cosmology. Part II. Initial conditions ⋮ Hi-COLA: fast, approximate simulations of structure formation in Horndeski gravity ⋮ A relativistic interpretation of bias in Newtonian simulations ⋮ General relativistic weak-field limit and Newtonian N-body simulations ⋮ fNL−gNL mixing in the matter density field at higher orders ⋮ Relativistic corrections to the growth of structure in modified gravity ⋮ fRevolution— relativistic cosmological simulations in f(R) gravity. Part I. Methodology
Uses Software
Cites Work
This page was built for publication: Relativistic initial conditions for N-body simulations
