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  • Open Access

Superrenormalizable hairy meronic black holes

Luis Avilés1,2,* and Borja Diez3,†

  • 1Instituto de Ciencias Exactas y Naturales, Universidad Arturo Prat, Playa Brava 3256, 1111346, Iquique, Chile
  • 2Facultad de Ciencias, Universidad Arturo Prat, Avenida Arturo Prat Chacón 2120, 1110939, Iquique, Chile
  • 3Departamento de Física, Cinvestav, Av. IPN 2508, 07360, CDMX, México

  • *Contact author: luaviles@unap.cl
  • †Contact author: borja.diez@cinvestav.mx

Phys. Rev. D 114, 024010 – Published 6 July, 2026

DOI: https://doi.org/10.1103/x32x-tjrz

Abstract

We construct an analytical black hole solution in the Einstein-Maxwell-Yang-Mills theory with a conformally coupled scalar field in four dimensions, which generalizes the charged Martínez-Troncoso-Zanelli (MTZ) black hole in the presence of self-gravitating non-Abelian gauge fields. The internal gauge group is determined by the horizon curvature, becoming SU(N) in the case of positive curvature and SU(N−1,1) when the curvature is negative. Moreover, this solution is employed as a conformal seed to obtain new meronic spacetimes dressed with all superrenormalizable contributions of the scalar field, which provides the generalization of the Anabalón-Cisterna solution when self–gravitating non-Abelian gauge fields are included. Finally, we consider the non-Noetherian extension of the conformal scalar fields, which still yields a second-order conformally invariant scalar equation, even though the action is not. In that case, we show that static black hole solutions can also be charged with Yang-Mills fields.

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