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A Four-Parameter Black-Hole Solution in the Bumblebee Gravity Model

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arxiv 2301.12666 v1 pith:ROXWSWSZ submitted 2023-01-30 gr-qc hep-ph

classification gr-qchep-ph
keywords solutionmodelblack-holebumblebeegravityparametersanalyticalchoices
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The bumblebee gravity model includes a class of vector-tensor theories of gravitation where the vector field couples to the Ricci tensor quadratically. We obtain an analytical spherical black-hole solution in this model. The solution has four parameters, expanding the two-parameter solution family known in the literature. Special choices of the parameters are pointed out and discussed.

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Cited by 1 Pith paper

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  1. Taub-NUT-like Black Holes in Einstein-Bumblebee Gravity

    gr-qc 2025-05 conditional novelty 4.0 of 10

    A new Taub-NUT-like black hole solution in Einstein-Bumblebee gravity is constructed, and its thermodynamics is shown to obey the first law and the Smarr relation.

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