Coordinate independent approach to the calculation of the effects of local structure on the luminosity distance
DOI10.1088/1475-7516/2020/03/023zbMath1490.85009arXiv1906.04946OpenAlexW3011071969MaRDI QIDQ5068418
Antonio Enea Romano, Sergio Andrés Vallejo-Peña
Publication date: 6 April 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1906.04946
Relativistic cosmology (83F05) Diffraction, scattering (78A45) NLS equations (nonlinear Schrödinger equations) (35Q55) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Electromagnetic fields in general relativity and gravitational theory (83C50) Perturbations in context of PDEs (35B20) Galactic and stellar structure (85A15) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Variational problems in applications to the theory of geodesics (problems in one independent variable) (58E10) Radiative transfer in astronomy and astrophysics (85A25) Mono-, di- and multipole moments (EM and other), gyromagnetic relations (81V60)
Cites Work
- Conditions for low-redshift positive apparent acceleration in smooth inhomogeneous models
- Spatial averaging and apparent acceleration in inhomogeneous spaces
- Redshift drift in varying speed of light cosmology
- Observational constraints on inhomogeneous cosmological models without dark energy
- INHOMOGENEOUS COSMOLOGICAL MODELS AND H0 OBSERVATIONS
- A new method to determine large scale structure from the luminosity distance
- Reconstructing the metric of the local Universe from number counts observations
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Spherically Symmetrical Models in General Relativity
- The expanding universe
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