Increasing the Lorentz-violating coefficient X in rotating bumblebee black holes causes teardrop deformations and flattening in their shadows, distinct from Kerr.
Gyoto: a new general relativistic ray-tracing code.Classical and Quantum Gravity, 28(22):225011
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Rotating black hole shadows in metric-affine bumblebee gravity
Increasing the Lorentz-violating coefficient X in rotating bumblebee black holes causes teardrop deformations and flattening in their shadows, distinct from Kerr.