Accurate relativistic observables from post-processing light cone catalogues

Abstract

We introduce and study a new scheme to construct relativistic observables from post-processing light cone data. This construction is based on a novel approach, LC-Metric, which takes general light cone or snapshot output generated by arbitrary N-body simulations or emulations and solves the linearized Einstein equations to determine the spacetime metric on the light cone. We find that this scheme is able to determine the metric to high precision, and subsequently generate accurate mock cosmological observations sensitive to effects such as post-Born lensing and nonlinear ISW contributions. By comparing to conventional methods in quantifying those general relativistic effects, we show that this scheme is able to accurately construct the lensing convergence signal. We also find the accuracy of this method in quantifying the ISW effects in the highly nonlinear regime outperforms conventional methods by an order of magnitude. This scheme opens a new path for exploring and modeling higher-order and nonlinear general relativistic contributions to cosmological observables, including mock observations of gravitational lensing and the moving lens and Rees-Sciama effects.

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Cited by in corpus (5)

• CosmoGridV1: a simulated $w$CDM theory prediction for map-level cosmological inference
• The halo bias for number counts on the light cone from relativistic N-body simulations
• Gauge invariance on the light-cone: curvature perturbations and radiative degrees of freedom
• Structure formation and quasi-spherical collapse from initial curvature perturbations with numerical relativity simulations
• $\delta N$ formalism on the past light-cone