Fractal universe and cosmic acceleration in a Lemaître–Tolman–Bondi scenario

DOI10.1088/1361-6382/AAE8F7zbMath1476.83185arXiv1810.06318OpenAlexW2897131169WikidataQ63391072 ScholiaQ63391072MaRDI QIDQ3380499

Leonardo Cosmai, Francesco Sylos Labini, Giuseppe Fanizza, Luciano Pietronero, Luigi Tedesco

Publication date: 29 September 2021

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1810.06318

zbMATH Keywords

fractal universeacceleration of the universeLemaitre-Tolman-Bondi scenario

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Galactic and stellar structure (85A15) Fractals (28A80)

Related Items (3)

On generalized Lemaitre–Tolman–Bondi metric: Fractal matter at the end of matter–antimatter recombination ⋮ A fractal LTB model cannot explain dark energy ⋮ Fractional cosmic strings

Cites Work

• Spatial averaging and apparent acceleration in inhomogeneous spaces
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• On average properties of inhomogeneous fluids in general relativity: Dust cosmologies
• Dark energy from structure: a status report
• Inhomogeneities in the universe
• Is there proof that backreaction of inhomogeneities is irrelevant in cosmology?
• Discriminating different models of luminosity–redshift distribution
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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