Cosmological distances with general-relativistic ray tracing: framework and comparison to cosmographic predictions
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Publication:6100397
DOI10.1088/1475-7516/2023/03/019zbMath1522.83446arXiv2209.06775OpenAlexW4323366138MaRDI QIDQ6100397
Publication date: 12 May 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2209.06775
Relativistic cosmology (83F05) Diffraction, scattering (78A45) Nonlinear higher-order PDEs (35G20) Gravitational energy and conservation laws; groups of motions (83C40) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)
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Cites Work
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- On the definition of distance in general relativity: I. M. H. Etherington (Philosophical Magazine ser. 7, vol. 15, 761 (1933))
- On average properties of inhomogeneous fluids in general relativity: Dust cosmologies
- On average properties of inhomogeneous fluids in general relativity. III: General fluid cosmologies
- The Einstein Toolkit: a community computational infrastructure for relativistic astrophysics
- Backreaction: directions of progress
- Gravitational waves in general relativity. VI. The outgoing radiation condition
- Inhomogeneity and the foundations of concordance cosmology
- Jerk, snap and the cosmological equation of state
- BiGONLight: light propagation with bilocal operators in numerical relativity
- Ray tracing and Hubble diagrams in post-Newtonian cosmology
- Light propagation through black-hole lattices
- General relativistic cosmological N-body simulations. Part I. Time integration
- A prediction for anisotropies in the nearby Hubble flow
- The Hubble series: convergence properties and redshift variables
- Multipole decomposition of the general luminosity distance Hubble law — a new framework for observational cosmology
- The averaging problem on the past null cone in inhomogeneous dust cosmologies
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