The type III stress-energy tensor: ugly duckling of the Hawking–Ellis classification

DOI10.1088/1361-6382/ab56f6zbMath1478.83072arXiv1907.01269OpenAlexW3105313811MaRDI QIDQ5161273

Prado Martín-Moruno, Matt Visser

Publication date: 29 October 2021

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

Full work available at URL: https://arxiv.org/abs/1907.01269

zbMATH Keywords

Kundt spacetimesgyratonHawking-Elllis classificationtype III stress-energy tensor

Mathematics Subject Classification ID

Semiclassical techniques, including WKB and Maslov methods applied to problems in quantum theory (81Q20) Gravitational energy and conservation laws; groups of motions (83C40) Motion of the gyroscope (70E05)

Related Items (4)

Energy conditions for non-timelike thin shells ⋮ Shadows of Kerr–Vaidya-like black holes ⋮ The Kiselev black hole is neither perfect fluid, nor is it quintessence ⋮ Nonstaticity with type II, III, or IV matter field in \(f(R_{\mu\nu\rho\sigma},g^{\mu\nu})\) gravity

Cites Work

• Four causal classes of Newtonian frames
• Hawking–Ellis type III spacetime geometry
• Essential core of the Hawking–Ellis types
• All solutions of Einstein’s equations in 2+1 dimensions: Λ-vacuum, pure radiation, or gyratons
• General Kundt spacetimes in higher dimensions
• Kundt spacetimes
• Exact Solutions of Einstein's Field Equations
• Generalized Rainich conditions, generalized stress–energy conditions, and the Hawking–Ellis classification
• All spacetimes with vanishing curvature invariants
• Classical and Semi-classical Energy Conditions
• Exact Space-Times in Einstein's General Relativity

This page was built for publication: The type III stress-energy tensor: ugly duckling of the Hawking–Ellis classification