pith. sign in

General relativistic weak-field limit and Newtonian N-body simulations

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

We show how standard Newtonian N-body simulations can be interpreted in terms of the weak-field limit of general relativity by employing the recently developed Newtonian motion gauge. Our framework allows the inclusion of radiation perturbations and the non-linear evolution of matter. We show how to construct the weak-field metric by combining Newtonian simulations with results from Einstein-Boltzmann codes. We discuss observational effects on weak lensing and ray tracing, identifying important relativistic corrections.

citation-role summary

background 1 method 1

citation-polarity summary

years

2026 2

verdicts

UNVERDICTED 2

clear filters

representative citing papers

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges

astro-ph.CO · 2026-05-06 · unverdicted · novelty 7.0 · 2 refs

A Newtonian Motion Gauge found via Einstein-Boltzmann solver maps linear dynamics with scale-dependent growth and GR corrections to Newtonian equations, enabling consistent nonlinear EFT calculations that are transformed back for accuracy in real and redshift space.

A Master Equation for Screening in Luminal Horndeski Gravity

gr-qc · 2026-05-05 · unverdicted · novelty 7.0

A master screening equation is derived for luminal Horndeski gravity that recovers Vainshtein and Chameleon mechanisms and introduces Phaedrus screening with screening radius scaling linearly with source mass.

citing papers explorer

Showing 2 of 2 citing papers.

  • Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges astro-ph.CO · 2026-05-06 · unverdicted · none · ref 9 · 2 links · internal anchor

    A Newtonian Motion Gauge found via Einstein-Boltzmann solver maps linear dynamics with scale-dependent growth and GR corrections to Newtonian equations, enabling consistent nonlinear EFT calculations that are transformed back for accuracy in real and redshift space.

  • A Master Equation for Screening in Luminal Horndeski Gravity gr-qc · 2026-05-05 · unverdicted · none · ref 84

    A master screening equation is derived for luminal Horndeski gravity that recovers Vainshtein and Chameleon mechanisms and introduces Phaedrus screening with screening radius scaling linearly with source mass.