Energy conditions for non-timelike thin shells
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Publication:6046928
DOI10.1088/1361-6382/acf181arXiv2306.07326OpenAlexW4385912856MaRDI QIDQ6046928
Publication date: 6 September 2023
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2306.07326
Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
- On the algebraic structure of second order symmetric tensors in 5-dimensional space-times
- Dynamics of anti-de Sitter domain walls
- Boundary terms and junction conditions for generalized scalar-tensor theories
- Israel conditions for the Gauss-Bonnet theory and the Friedmann equation on the brane universe
- Segre types of symmetric two-tensors in \(n\)-dimensional spacetimes
- Creation of Wormholes by First Order Phase Transition of a Vacuum in the Early Universe
- All solutions of Einstein’s equations in 2+1 dimensions: Λ-vacuum, pure radiation, or gyratons
- Inner structure of a charged black hole: An exact mass-inflation solution
- Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- A Relativist's Toolkit
- Classification of second order symmetric tensors in five-dimensional Kaluza–Klein-type theories
- Energy conditions in arbitrary dimensions
- The type III stress-energy tensor: ugly duckling of the Hawking–Ellis classification
- Junction conditions in scalar–tensor theories
- Gravitation
- Classical and Semi-classical Energy Conditions
- Avoiding closed timelike curves with a collapsing rotating null dust shell
- The Large Scale Structure of Space-Time
- Black-bounce to traversable wormhole
- Criteria for energy conditions
- Brane-world cosmology
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