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This paper reveals a new black hole model involving a scalar field and provides thermodynamic insights.
This paper presents a new four-dimensional axionic-charged rotating black hole with a scalar field, which is defined by a structural function coupling the axionic field and a scalar potential. This configuration is characterized by an integration constant and two parameters. The thermodynamic parameters are obtained via the Euclidean procedure, where the validity of the first law of thermodynamics is ensured. With the above information, we can see that this rotating configuration is a good laboratory from the perspective of the holographic superconductor, in which the angular parameter plays an important role.
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Bravo‐Gaete et al. (2025) studied this question.
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