A weak acceleration effect due to residual gravity in a multiply connected universe

DOI10.1051/0004-6361:20064979zbMath1118.85330arXivastro-ph/0602159OpenAlexW1984471631WikidataQ68598777 ScholiaQ68598777MaRDI QIDQ5292937

A. Szaniewska, Boudewijn François Roukema, Marek Biesiada, H. Jurkiewicz, Stanisław Bajtlik

Publication date: 25 June 2007

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

Full work available at URL: https://arxiv.org/abs/astro-ph/0602159

zbMATH Keywords

gravitationcosmology theorycosmology cosmological parameters

Mathematics Subject Classification ID

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

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

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