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Bibliographic Details
Main Authors: Avilés, Luis, Valdivia, Omar, Véliz, Rodolfo, Vera, Carlos
Format: Preprint
Published: 2026
Subjects:
Online Access:https://arxiv.org/abs/2605.26360
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author Avilés, Luis
Valdivia, Omar
Véliz, Rodolfo
Vera, Carlos
author_facet Avilés, Luis
Valdivia, Omar
Véliz, Rodolfo
Vera, Carlos
contents We formulate a one-parameter extension of Weyl transformations in first-order gravity and show that it defines a conformally coupled scalar sector with dynamical torsion. The construction reduces to the standard torsionless conformal coupling in the limit $λ\to 1$. In the corresponding Einstein-Cartan-Maxwell theory, we derive exact static solutions in asymptotically flat and asymptotically locally AdS spacetimes. These solutions describe scalar-dressed black holes, regular black holes, and traversable wormholes, depending on the values of the integration constants and of the deformation parameter. We show that torsion can regularize the scalar field and, for suitable branches, also improve the geometric singularity structure. In the AdS sector, the existence of topological black holes requires a nonvanishing electric charge. These results provide new exact examples of regular and torsional configurations in four-dimensional gravity.
format Preprint
id arxiv_https___arxiv_org_abs_2605_26360
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Torsional black holes and wormholes in Einstein-Cartan-Maxwell gravity with a conformal scalar field
Avilés, Luis
Valdivia, Omar
Véliz, Rodolfo
Vera, Carlos
High Energy Physics - Theory
We formulate a one-parameter extension of Weyl transformations in first-order gravity and show that it defines a conformally coupled scalar sector with dynamical torsion. The construction reduces to the standard torsionless conformal coupling in the limit $λ\to 1$. In the corresponding Einstein-Cartan-Maxwell theory, we derive exact static solutions in asymptotically flat and asymptotically locally AdS spacetimes. These solutions describe scalar-dressed black holes, regular black holes, and traversable wormholes, depending on the values of the integration constants and of the deformation parameter. We show that torsion can regularize the scalar field and, for suitable branches, also improve the geometric singularity structure. In the AdS sector, the existence of topological black holes requires a nonvanishing electric charge. These results provide new exact examples of regular and torsional configurations in four-dimensional gravity.
title Torsional black holes and wormholes in Einstein-Cartan-Maxwell gravity with a conformal scalar field
topic High Energy Physics - Theory
url https://arxiv.org/abs/2605.26360