The residual gravity acceleration effect in the Poincaré dodecahedral space

DOI10.1051/0004-6361/200911881zbMath1177.85087arXiv0902.3402OpenAlexW2142890946WikidataQ68676519 ScholiaQ68676519MaRDI QIDQ3639170

Unnamed Author, Boudewijn François Roukema

Publication date: 29 October 2009

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0902.3402

zbMATH Keywords

early universecosmological parameterslarge-scale structure of universecosmology: theory

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Astrophysical cosmology (85A40)

Related Items (4)

DOES GRAVITY PREFER THE POINCARÉ DODECAHEDRAL SPACE? ⋮ On non-Euclidean Newtonian theories and their cosmological backreaction ⋮ Gauss–Bonnet–Chern approach to the averaged Universe ⋮ The spectral action and cosmic topology

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