Smooth and discontinuous signature type change in general relativity
From MaRDI portal
Publication:4280454
DOI10.1088/0264-9381/10/11/019zbMath0791.53064OpenAlexW2036363125MaRDI QIDQ4280454
Marcus Kriele, Marek Kossowski
Publication date: 18 July 1994
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1088/0264-9381/10/11/019
Space-time singularities, cosmic censorship, etc. (83C75) Global differential geometry of Lorentz manifolds, manifolds with indefinite metrics (53C50)
Related Items (21)
Classical and quantum implications of the causality structure of two-dimensional space–times with degenerate metrics ⋮ CASIMIR EFFECT FOR A SPHERICAL SHELL IN DE SITTER SPACE–TIME WITH SIGNATURE CHANGE ⋮ Solvability theorems for linear equations of Tricomi type ⋮ Euclidean action, nucleation energy and the dimensionality of space-time ⋮ Topology change and the propagation of massless fields ⋮ Metric singularities ⋮ Isochronous solutions of Einstein’s equations and their Newtonian limit ⋮ Comment on: ``Smooth and discontinuous signature change in general relativity ⋮ Reply to: Comment on ``Smooth and discontinuous signature type change in GR ⋮ Propagation of singularities phenomena for equations of tricome type ⋮ CASIMIR STRESS ON PARALLEL PLATES IN DE SITTER SPACE WITH SIGNATURE CHANGE ⋮ Note on signature change and Colombeau theory ⋮ Casimir effect for concentric spheres in de Sitter spacetime with signature change ⋮ Singularities of the geodesic flow on surfaces with pseudo-Riemannian metrics ⋮ Einstein’s equations in the presence of signature change ⋮ Mixed type surfaces with bounded Gaussian curvature in three-dimensional Lorentzian manifolds ⋮ On singular semi-Riemannian manifolds ⋮ Tensor distributions on signature-changing space-times ⋮ New junction conditions for signature change: null boundary proposal ⋮ Isochronous spacetimes ⋮ ON SIGNATURE TRANSITION IN ROBERTSON–WALKER COSMOLOGIES
This page was built for publication: Smooth and discontinuous signature type change in general relativity
