Nonexistence of closed timelike geodesics in Kerr spacetimes
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Publication:6597612
DOI10.1063/5.0221959zbMATH Open1545.83134MaRDI QIDQ6597612
Publication date: 3 September 2024
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Applications of differential geometry to physics (53Z05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Geodesics in global differential geometry (53C22)
Cites Work
- Title not available (Why is that?)
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- Spherical photon orbits around a Kerr black hole
- Über das Gravitationsfeld eines Massenpunktes nach der \textit{Einstein}schen Theorie.
- On quadratic first integrals of the geodesic equations for type [22] spacetimes
- THE GEODESICS IN GÖDEL'S UNIVERSE
- Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
- Particle motion near high-spin black holes
- Causality violation without time-travel: closed lightlike paths in Gödel’s universe
- Maximal Analytic Extension of the Kerr Metric
- Global Structure of the Kerr Family of Gravitational Fields
- An Example of a New Type of Cosmological Solutions of Einstein's Field Equations of Gravitation
- Nonexistence of closed and bounded null geodesics in Kerr spacetimes
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