Is a topology change after a Big Rip possible?

DOI10.1142/S0219887819500488zbMath1426.83056arXiv1805.11945OpenAlexW2807044758MaRDI QIDQ5232404

V. K. Oikonomou

Publication date: 3 September 2019

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1805.11945

zbMATH Keywords

topology changebig ripfinite time singularitiescosmic singularities

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Completely integrable finite-dimensional Hamiltonian systems, integration methods, integrability tests (37J35) Space-time singularities, cosmic censorship, etc. (83C75) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Geodesics in global differential geometry (53C22) Galactic and stellar dynamics (85A05)

Related Items (1)

Finite-time cosmological singularities and the possible fate of the universe

Cites Work

• Shocks and finite-time singularities in Hele-Shaw flow
• Selection rules for topology change
• Phase transitions and configuration space topology
• Loop quantum cosmology: a status report
• Kinks and topology change
• The singularities of gravitational collapse and cosmology
• Gravitational Collapse and Space-Time Singularities
• Unnamed Item

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