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A Four-Parameter Black-Hole Solution in the Bumblebee Gravity Model
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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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Taub-NUT-like Black Holes in Einstein-Bumblebee Gravity
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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