Essential core of the Hawking–Ellis types

DOI10.1088/1361-6382/aac147zbMath1391.83039arXiv1802.00865OpenAlexW2787684080WikidataQ59619419 ScholiaQ59619419MaRDI QIDQ3177425

Prado Martín-Moruno, Matt Visser

Publication date: 25 July 2018

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1802.00865

zbMATH Keywords

energy conditionsHawking-Ellis typestress-energy classification

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Gravitational energy and conservation laws; groups of motions (83C40)

Related Items (8)

The eye of the storm: a regular Kerr black hole ⋮ A connection between regular black holes and horizonless ultracompact stars ⋮ Feynman's \(i\epsilon\) prescription, almost real spacetimes, and acceptable complex spacetimes ⋮ Observer-based invariants for cosmological models ⋮ 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 ⋮ Hawking–Ellis type III spacetime geometry ⋮ Charged black-bounce spacetimes

Cites Work

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• Classical and Semi-classical Energy Conditions
• The spacetime geometry of a null electromagnetic field
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• Geometrization conditions for perfect fluids, scalar fields, and electromagnetic fields
• The Large Scale Structure of Space-Time

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