Bumblebee gravity parameters ℓ and Q shrink central dark regions, enhance brightness asymmetry, and alter polarization patterns in thick-disk images of Kerr-Sen-like black holes.
0.5 1.0 (b)Stokes parameterQ o -8 -4 0 4 8 -8 -4 0 4 8 x y -1.0 -0.5 0
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Imprints of Black Hole Shadows and Polarization Patterns of Various Thick Disks: Bumblebee gravity
Bumblebee gravity parameters ℓ and Q shrink central dark regions, enhance brightness asymmetry, and alter polarization patterns in thick-disk images of Kerr-Sen-like black holes.