For ultracompact black hole mimickers, the polar magnetic field is predicted to be weaker than the equatorial field by a factor of roughly z_s/ln z_s, a signature that could observationally separate horizonless mimickers from true black holes.
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How to distinguish an actual astrophysical magnetized black hole mimicker from a true (theoretical) black hole
For ultracompact black hole mimickers, the polar magnetic field is predicted to be weaker than the equatorial field by a factor of roughly z_s/ln z_s, a signature that could observationally separate horizonless mimickers from true black holes.