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Kerr black holes with synchronised scalar hair and higher azimuthal harmonic index

2 Pith papers cite this work. Polarity classification is still indexing.

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abstract

Kerr black holes with synchronised scalar hair and azimuthal harmonic index $m>1$ are constructed and studied. The corresponding domain of existence has a broader frequency range than the fundamental $m=1$ family; moreover, larger ADM masses, $M$ and angular momenta $J$ are allowed. Amongst other salient features, non-uniqueness of solutions for fixed global quantities is observed: solutions with the same $M$ and $J$ co-exist, for consecutive values of $m$, and the ones with larger $m$ are always entropically favoured. Our analysis demonstrates, moreover, the qualitative universality of various features observed for $m=1$ solutions, such as the shape of the domain of existence, the typology of ergo-regions, and the horizon geometry, which is studied through its isometric embedding in Euclidean 3-space.

fields

gr-qc 2

years

2026 1 2025 1

verdicts

UNVERDICTED 2

representative citing papers

Distorting Kerr Images with Parity-Odd Scalar Hair

gr-qc · 2026-05-27 · unverdicted · novelty 5.0

Numerical study of thin accretion disk images shows that increasing parity-odd scalar hair on Kerr black holes shrinks and distorts the photon ring and shadow, producing multiple disconnected shadows and chaotic lensing features in strong-hair regimes.

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