ORIGINAL RESEARCH article
Front. Astron. Space Sci.
Sec. Cosmology
Volume 12 - 2025 | doi: 10.3389/fspas.2025.1675093
This article is part of the Research TopicBlack Hole Physics in Modified Gravity TheoriesView all articles
Regular Bardeen-like Black Holes in Higher-Dimensional Pure Lovelock Gravity with Nonlinear Yang-Mills Fields
Provisionally accepted- Eastern Mediterranean University, Famagusta, Türkiye
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We construct spherically symmetric, static, and regular Bardeen-like black hole solutions in the framework of higher-dimensional pure Lovelock gravity coupled to nonlinear Yang-Mills fields. The gauge fields are modeled using a higher-dimensional Wu-Yang ansatz, and the nonlinear Lagrangian is designed to resemble the Bardeen-type black holes in Einstein gravity. The resulting solutions are asymptotically flat and regular at the origin, with curvature invariants remaining finite throughout the spacetime. We show that in dimensions N = 2p + 1, the solutions describe particle-like con-figurations without horizons. However, for N > 2p + 1, depending on the model parameters, the solutions can represent either regular black holes or particle-like spacetimes. We derive analytic con-ditions that determine the horizon structure and classify the spacetime accordingly. Furthermore, we perform a detailed analysis of the thermal stability of the black holes by computing the Hawking temperature and heat capacity. The thermodynamic phase structure reveals regions of stability and the presence of both first-and second-order phase transitions. Our results extend the concept of regular black holes to the setting of pure Lovelock gravity and highlight the rich interplay between nonlinearity, dimensionality, and gauge dynamics.
Keywords: Regular Bardeen-like Black Holes, Higher-Dimensional Pure Lovelock Gravity, Nonlinear Yang-Mills Fields, Spherically symmetric, static, regular Bardeen-like black hole solutions, higher-dimensional Wu-Yang ansatz, Asymptotically flat
Received: 28 Jul 2025; Accepted: 18 Sep 2025.
Copyright: © 2025 Mazharimousavi. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
* Correspondence: S. Habib Mazharimousavi, habib.mazhari@emu.edu.tr
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