Spinning generalizations of Majumdar-Papapetrou multi-black-hole spacetimes: Light rings, lensing, and shadows

A generalization of the Majumdar-Papapetrou multi-black-hole spacetime was recently constructed by Teo and Wan [Phys. Rev. D 109, 044054 (2024)], describing charged and spinning (extremal) balanced black holes in asymptotically flat spacetime. We explore the dynamics of null geodesics on this geometry, focusing on the two-center solution. Using the topological charge formalism, we show that various light ring arrangements arise from different choices of individual angular momenta: light rings with opposite topological charges can merge and annihilate each other, resulting in configurations with a total of 4, 6, or 8 light rings. Using backward ray tracing, we obtained the shadow and lensing of these spacetimes. The former, in particular, closely resembles those for the double Kerr metric.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-04-01
DOI
https://doi.org/10.1103/physrevd.111.084002
Citations
1
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
1.15

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article

Spinning generalizations of Majumdar-Papapetrou multi-black-hole spacetimes: Light rings, lensing, and shadows

Carlos Herdeiro, Zeus S. Moreira, Luís C. B. Crispino
1 citations
Physical review. D/Physical review. D.
Astrophysical Phenomena and Observations
1.15
article

Spinning generalizations of Majumdar-Papapetrou multi-black-hole spacetimes: Light rings, lensing, and shadows

Carlos Herdeiro, Zeus S. Moreira, Luís C. B. Crispino
article en
1 citations

Abstract

A generalization of the Majumdar-Papapetrou multi-black-hole spacetime was recently constructed by Teo and Wan [Phys. Rev. D 109, 044054 (2024)], describing charged and spinning (extremal) balanced black holes in asymptotically flat spacetime. We explore the dynamics of null geodesics on this geometry, focusing on the two-center solution. Using the topological charge formalism, we show that various light ring arrangements arise from different choices of individual angular momenta: light rings with opposite topological charges can merge and annihilate each other, resulting in configurations with a total of 4, 6, or 8 light rings. Using backward ray tracing, we obtained the shadow and lensing of these spacetimes. The former, in particular, closely resembles those for the double Kerr metric.

Physical review. D/Physical review. D.Vol. 111(8)
Universidade Federal do Pará (BR)
Coordenação de Aperfeiçoamento de Pessoal de Nível Superior, Conselho Nacional de Desenvolvimento Científico e Tecnológico, Fundação Amazônia Paraense de Amparo à Pesquisa, Center for Research and Development in Mathematics and Applications, Fundação para a Ciência e a Tecnologia, HORIZON EUROPE Marie Sklodowska-Curie Actions
Openalex Percentile: Top 20%
Astrophysical Phenomena and Observations
1.15
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