Ray tracing and Hubble diagrams in post-Newtonian cosmology

DOI10.1088/1475-7516/2017/07/028OpenAlexW3102214758MaRDI QIDQ5019981

Viraj A. A. Sanghai, Pierre Fleury, Timothy Clifton

Publication date: 11 January 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1705.02328

zbMATH Keywords

cosmological simulationscosmological parameters from LSS

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items

The effect of dark matter discreteness on light propagation ⋮ Cosmological distances with general-relativistic ray tracing: framework and comparison to cosmographic predictions ⋮ The averaging problem on the past null cone in inhomogeneous dust cosmologies ⋮ Cosmological solutions with charged black holes ⋮ Cosmic expansion from spinning black holes ⋮ Black-hole lattices as cosmological models ⋮ A quasi-static approach to structure formation in black hole universes ⋮ Optical drift effects in general relativity ⋮ Second-order dust perturbations of the non-flat FLRW model with the positive cosmological constant

Uses Software

• gevolution

Cites Work

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