Geodesics with negative energy in the ergosphere of rotating black holes

DOI10.1142/S0217732314501107zbMath1295.83040arXiv1304.7360MaRDI QIDQ2879217

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Publication date: 8 September 2014

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1304.7360

zbMATH Keywords

black holegeodesicKerr metric

Mathematics Subject Classification ID

Black holes (83C57) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (11)

High energy physics in the vicinity of rotating black holes ⋮ Super-Penrose process for extremal rotating neutral white holes ⋮ Naked singularity formation in generalized Vaidya space-time ⋮ High-energy collision of particles in the magnetic field far from black holes ⋮ Geodesics for particles with negative energy in Kerr's metric ⋮ Comparison of particle properties in Kerr metric and in rotating coordinates ⋮ Equatorial geodesics in ergoregion of dirty black holes and zero energy observers ⋮ Black holes and particles with zero or negative energy ⋮ Are black holes totally black? ⋮ On geodesics with negative energies in the ergoregions of dirty black holes ⋮ Internal structures and circular orbits for test particles

Cites Work

• Unnamed Item
• Orbits through the ergosphere of a Kerr black hole
• PARTICLES WITH NEGATIVE ENERGIES IN BLACK HOLES
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• Maximal Analytic Extension of the Kerr Metric
• Global Structure of the Kerr Family of Gravitational Fields
• The Large Scale Structure of Space-Time
• General Relativity

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