Classical and Semi-classical Energy Conditions
From MaRDI portal
Publication:5355216
DOI10.1007/978-3-319-55182-1_9zbMath1370.83022arXiv1702.05915OpenAlexW2592828276MaRDI QIDQ5355216
Prado Martín-Moruno, Matt Visser
Publication date: 7 September 2017
Published in: Fundamental Theories of Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1702.05915
Related Items (20)
A singularity theorem for Einstein-Klein-Gordon theory ⋮ Conformally Schwarzschild cosmological black holes ⋮ Essential core of the Hawking–Ellis types ⋮ Thakurta metric does not describe a cosmological black hole ⋮ Energy conditions for non-timelike thin shells ⋮ Feynman's \(i\epsilon\) prescription, almost real spacetimes, and acceptable complex spacetimes ⋮ Dominant energy condition and dissipative fluids in general relativity ⋮ The quantum null energy condition in curved space ⋮ Generalized Rainich conditions, generalized stress–energy conditions, and the Hawking–Ellis classification ⋮ Vaidya spacetimes, black-bounces, and traversable wormholes ⋮ The type III stress-energy tensor: ugly duckling of the Hawking–Ellis classification ⋮ The Kiselev black hole is neither perfect fluid, nor is it quintessence ⋮ New perspectives on the TOV equilibrium from a dual null approach ⋮ Energy conditions in general relativity and quantum field theory ⋮ Phantom singularities and their quantum fate: general relativity and beyond -- a CANTATA COST action topic ⋮ All solutions of Einstein’s equations in 2+1 dimensions: Λ-vacuum, pure radiation, or gyratons ⋮ Hawking–Ellis type III spacetime geometry ⋮ Black-bounce to traversable wormhole ⋮ Criteria for energy conditions ⋮ Charged black-bounce spacetimes
This page was built for publication: Classical and Semi-classical Energy Conditions