Increasing the Lorentz-violating coefficient X in rotating bumblebee black holes causes teardrop deformations and flattening in their shadows, distinct from Kerr.
Deflection angle in the strong deflection limit in a general asymptotically flat, static, spherically symmetric spacetime.Phys
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
citation-role summary
method 1
citation-polarity summary
fields
gr-qc 1years
2026 1verdicts
UNVERDICTED 1roles
method 1polarities
use method 1representative citing papers
citing papers explorer
-
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.