Classical Signature Change in the Black Hole Topology

DOI10.1142/S0218271897000133zbMath0936.83031arXivgr-qc/9907042OpenAlexW1975312391MaRDI QIDQ4936959

Charles Hellaby, Ariel Sumeruk, George F. R. Ellis

Publication date: 2 February 2000

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

Full work available at URL: https://arxiv.org/abs/gr-qc/9907042

zbMATH Keywords

signature changewave function of the universebounce

Mathematics Subject Classification ID

Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (6)

Can black holes have Euclidean cores? ⋮ Revisiting the Darmois and Lichnerowicz junction conditions ⋮ Variational equations on mixed Riemannian-Lorentzian metrics ⋮ Nondifferentiable dynamics: Two examples ⋮ On fractional and fractal Einstein’s field equations ⋮ Geodesic family of spherical instantons and cosmic quantum creation

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