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We argue that black holes admit vortex structure.
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Such interactions are easily implementable in SU ( N ) (N) -saturon models with χ ± \chi_{\pm} transforming in appropriate representations of SU ( N ) (N)
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Note that an accretion disk might influence the BZ emission
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G. Dvali and O. Sakhelashvili, (2021), arXiv:2111.03620 [hep-th]
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