https://doi.org/10.1140/epjc/s10052-025-14567-2
Regular Article - Theoretical Physics
Rotating scalarized supermassive black holes
1
Center for Gravitation and Cosmology, College of Physical Science and Technology, Yangzhou University, 225009, Yangzhou, China
2
School of Mathematical Sciences, Qufu Normal University, 273165, Qufu, Shandong, China
3
Department of Physics and Siyuan Laboratory, Jinan University, 510632, Guangzhou, China
Received:
28
May
2025
Accepted:
18
July
2025
Published online:
2
August
2025
In this study, we investigate rotating black hole solutions within a scalar-Gauss–Bonnet gravity framework that incorporates a squared Gauss–Bonnet term. By employing a quadratic–exponential coupling function between the scalar field and the Gauss–Bonnet invariant, we derive both the standard General Relativity solutions and novel scalarized black hole configurations. Utilizing a pseudo-spectral method to solve the coupled field equations, we examine how black hole spin and coupling constants influence the existence and properties of these solutions. Our findings reveal that both the rotation of the black hole and the squared coupling term effectively constrain the parameter space available for scalarization. Moreover, we demonstrate that, over a wide range of parameters, scalarized black holes exhibit higher entropy than Kerr black holes of equivalent mass and spin, indicating that they are thermodynamically favored. These results significantly expand the phase space of black holes in modified gravity theories.
© The Author(s) 2025
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